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  <url>
    <loc>http://www.physicsmatt.com/blog</loc>
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    <lastmod>2025-12-12</lastmod>
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      <image:title>PhysicsMatt's Blog</image:title>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2025/12/11/paper-explainer-clearpotential-revealing-local-dark-matter-in-three-dimensions</loc>
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    <lastmod>2025-12-12</lastmod>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: ClearPotential: Revealing Local Dark Matter in Three Dimensions - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2025/12/11/the-dumbest-thing-ive-seen-this-week</loc>
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    <priority>0.5</priority>
    <lastmod>2025-12-16</lastmod>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2025/3/3/paper-explainer-general-constraints-on-isocurvature-from-the-cmb-and-ly-alpha-forest</loc>
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    <priority>0.5</priority>
    <lastmod>2025-03-04</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/bc7f93c6-4b2c-4633-9bdb-ab5699579219/final_limits_DR.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: General Constraints on Isocurvature from the CMB and Ly-alpha Forest - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/48472828-834a-4d69-8599-e179c46176b2/final_limits_Matter.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: General Constraints on Isocurvature from the CMB and Ly-alpha Forest - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/63f58eae-cde1-4491-9449-fb2c77fc6357/final_limits_Neutrino.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: General Constraints on Isocurvature from the CMB and Ly-alpha Forest - Make it stand out</image:title>
      <image:caption>Isocurvature limits for dark radiation (top), cold dark matter and baryons (middle), and neutrinos (bottom) assuming single-wavenumber isocurvature (left) or broken-power-law (right)</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2025/2/24/new-jersey-scholars-letter-on-the-threats-to-higher-education</loc>
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    <priority>0.5</priority>
    <lastmod>2025-02-24</lastmod>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2024/12/20/paper-explainer-mapping-dark-matter-through-the-dust-of-the-milky-way-part-i</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-12-20</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/efbc78c9-fc76-44a4-95c4-d24364c9643b/Gaia_s_sky_in_colour_pillars.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>The Milky Way (and LMC and SMC) as seen by Gaia. At high resolution, you can see that every dot in this image is an individual star. Image from ESA.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/c97e2838-a373-4617-a42b-113920c41bde/potw2114a.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>Spiral Galaxy M61. the spirals contain many bright young stars which are hot and blue (also star forming regions containing hydrogen gas which glows a reddish-pink). these disequilibrium structures are not reflected in the older less-blue population of stars.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/baeebb13-3b70-4d83-bc02-4038f311530d/BPRP_VS_MG_pre_post_L22_dust_correction_0.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>The stars with full velocity measurement within 4 kpc of the Sun, as seen by Gaia. The horizontal axis is “color” (red to the right, blue to the left). Vertical axis is intrinsic magnitude, brighter stars at the top. Below the horizontal dashed line, the stars are too dim to be seen by gaia if they are at the edge of the 4 kpc volume. The white square selects stars in the Red Clump.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/55bd8852-a536-4bc3-b3bd-9885460dff46/mass_density_measurement_no_bias_correction_full_panel.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>Mass density measured below and above the solar location, with the average dark matter mass density in the lower panel. From our previous work.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/a9ec4a47-023d-49f6-8658-a889a2df20b5/data_with_dust_labels_hires.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>Map of the well-measured bright stars we use in this work, from Gaia data. Known dust features are labeled.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/844bc8bd-65d5-48a3-9538-4d1aba215860/px_dist_3.00.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/981a5364-a3b0-4f04-825a-c7f9eefda146/pxTrue_dist_3.00.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/7e42ea86-705d-4d00-9edf-b57d2f77ec1c/L22_dustmap_eps_dist_2.00.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>The efficiency function as extrapolated from known dustmaps</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/4bdc8c8e-1473-46e3-805d-50ce88c4a06f/eps_dist_2.00.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Mapping Dark Matter Through the Dust of the Milky Way Part I - Make it stand out</image:title>
      <image:caption>The Efficiency function as learned by our network</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2024/10/29/paper-explainer-inferring-the-morphology-of-the-galactic-center-excess-with-gaussian-processes</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-10-30</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/d7b556de-8eb7-4b57-9505-64c1230c2ced/tim_models.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Theory space of dark matter models, by Tim Tait (2013)</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/0db1d7ad-5579-4059-af98-722db36a86c8/fig_allsky_data.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Gamma ray sky as seen by Fermi (Ramirez et al, 2024)</image:caption>
    </image:image>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes</image:title>
    </image:image>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes</image:title>
    </image:image>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/0281d6fa-f6cf-4478-8205-448961cc6440/fig_allsky_data_inset.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Inner Region of interest before any point source and disk masking (left), with masking (center), and including outer ROI (right). Ramirez et al 2024</image:caption>
    </image:image>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Results of SVI on synthetic data, showing we can recover the true parameters (red) from our analysis chain. Ramirez et al 2024</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/bcc86a5c-c21d-42ed-9137-5da1358641ed/fig_fit_to_data_all_models.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Gaussian Process fit to the Galactic Center Excess with background modeled by linear combination of 80 templates. Ramirez et al (2024)</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/fc5f4542-b7db-43cd-924c-6ccc953c4daa/fig_fit_to_data_bulge_comparisons.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Inferring the Morphology of the Galactic Center Excess with Gaussian Processes - Make it stand out</image:title>
      <image:caption>Preference for various known bulge components when NFW-squared profile is allowed fully flexible model parameters. Ramirez et al (2024).</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2024/10/8/paper-explainer-force-feeding-supermassive-black-holes-with-dissipative-dark-matter</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-10-10</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/996554c0-3ba5-4e41-a333-58b39e8d1a1f/example_coolingTrho.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Force-feeding Supermassive Black Holes with Dissipative Dark Matter - Make it stand out</image:title>
      <image:caption>Whatever it is, the way you tell your story online can make all the difference.</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2024/2/21/paper-explainer-dark-radiation-isocurvature-from-cosmological-phase-transitions</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-02-22</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/c0776d42-bce4-4b7f-9ed9-75725a6abd22/Planck_CMB_pillars.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Dark Radiation Isocurvature from Cosmological Phase Transitions - Make it stand out</image:title>
      <image:caption>Map of the Cosmic Microwave Background sky temperature perturbations, Planck (ESA)</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1b2c6c25-3caa-43ba-8d31-b24b55222bef/Schematic_scale.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Dark Radiation Isocurvature from Cosmological Phase Transitions - Make it stand out</image:title>
      <image:caption>Schematic of our Bubble nucleation during inflation and after (From Buckley et al)</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/4f5ac6b6-3fcc-49c4-a9f2-d04103250525/bubbles_Ht_4.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Dark Radiation Isocurvature from Cosmological Phase Transitions - Make it stand out</image:title>
      <image:caption>Simulation of Bubble nucleation during inflation. Earlier bubbles end up larger.</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2021/4/26/paper-explainer-via-machinae</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-10-09</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619491140327-NVQ1MLD72MMEIZNM4P4R/GD1_patch_allstars_notag.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
      <image:caption>“Via Machinae: Searching for Stellar Streams using Unsupervised Machine Learning” D. Shih, M.R. Buckley, L. Necib, J. Tamanas</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619491482879-X2YLP9TLRHF5BXVY9XN2/GD1_patch_allstars.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619491988523-KR1SH4XQPE5X1LPBTAKI/GD1_patch_allSR_Randsic_unstacked.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619492178085-HHRI5Z3TI5YM5BPOJBTK/GD1_patch_SRall_stars.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619492238850-2P3ALTSN4PRR29IA0IDL/GD1_patch_SR_rcut.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619492792089-RYX7WEPKRDYV5KYRQPFR/ViaMachinaeSchematicv4.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1619493394900-BNPZG7OH7UTI02BEQZEN/mockstream_combined.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
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    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Via Machinae</image:title>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2020/3/18/simulating-a-galaxy-without-a-computer</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2020-03-19</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1584588099480-KRLSIFJVX55PB4D27CZ3/SDSS.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>The cosmic web of galaxies as seen by SDSS.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1584587841997-Q49NSA6OD76I964B96JD/seqD_063a_half.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>Cosmic Web of dark matter from the Millennium simulation, tracing the location of matter in the Universe.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1584588897859-EMLAO8KTY6WI4AH515DF/holmberg_light.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>Schematic of the lightbulb and light sensor from Holmberg, E., Astrophysical Journal, vol. 94, p.385</image:caption>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>Initial conditions of one of the galaxies in th Holmberg Simulation From Holmberg, E., Astrophysical Journal, vol. 94, p.385</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1584589017214-JXMKYTQT5A61K1BLDUOM/holmberg_tides.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>Tidal tails of two interacting galaxies from Holmberg, E. Astrophysical Journal, vol. 94, p.385</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1584589116234-K3ALROH4L40D9451IFYJ/227982main_print_full.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Simulating a galaxy without a computer</image:title>
      <image:caption>Tidal tails of the Antennae Galaxies (NASA, ESA, The Hubble Heritage Collaboration)</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2019/7/1/applying-liouvilles-theorem-to-gaia-data</loc>
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    <priority>0.5</priority>
    <lastmod>2019-07-03</lastmod>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Cartoon of the structure of dark matter objects. From Buckley and Peter</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1562032210955-3MLWNHPVQVYIGHM96O93/movie.gif</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Simulation of a stream forming from a Globular Cluster in the Milky Way (galaxy center marked with Gold star).</image:caption>
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    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1562072197978-Z0Q2KM8S9DFCZ3OKJ5D0/Messier-4.jpg</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>M4 Globular Cluster, NASA/ESA Hubble</image:caption>
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    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Simulated stars in a M4-like globular cluster. Color and size of each star represent the relative phase space-density (larger points are lower density).</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1562072798102-159CAUOGHUA2WLLKGBG1/M4simulated_scatter_foregrounderrors.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Simulated stars in a M4-like globular cluster including measurement errors and foreground stars. Color and size of each star represent the relative phase space-density (larger points are lower density).</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1562072825453-OXGYH1TJHU1Q5TNT8CUL/M4simulated_scatter_foregrounderrors_cut.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Simulated stars in a M4-like globular cluster including measurement errors and foreground stars, after a cut on stars with large errors is applied. Color and size of each star represent the relative phase space-density (larger points are lower density).</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Best-fit mass and King profile radius for simulated M4 globular cluster, after cutting stars with large velocity errors. Correct answer is shown with the gold star, best-fit is the black star.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Best-fit mass and King profile radius for simulated M4 globular cluster, after cutting stars with large velocity errors and correcting for entropy-injection. Correct answer is shown with the gold star, best-fit is the black star.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Stars in the Gaia data set for the M4 globular cluster. Color and size of each star represent the relative phase space-density (larger points are lower density).</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Stars in the Gaia data set for the M4 globular cluster after a cut on the stars with large errors. Color and size of each star represent the relative phase space-density (larger points are lower density).</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Measurement of mass and King Radius for the M4 globular cluster using Gaia Data. Best-fit value of phase-space density technique is shown with black star, accepted best-fit value for the cluster is shown with a gold star.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Orbits of stars from a globular cluster (initial positions in red) as it is tidally disrupted in a simulation of the Milky Way. Blue dots are the locations of the stars after 500 million years. The future orbits of the stars over the next 500 million years (in the assumed Milky Way potential) are shown in gold. 10 sets of orbits assuming incorrect orbits are shown in black.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Applying Liouville's Theorem to Gaia Data</image:title>
      <image:caption>Entropy S of the phase-space densities of stars in a simulated stream for 1000 iterations of the Milky Way POtential versus the Kullback-Leiblier test statistic (a measure of how similar the Iterated potential is to the real potential). Note that the real potential has the minimum entropy, and that there is a trend of more similar potentials having lower entropies.</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2019/6/17/terrible-ideas</loc>
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    <lastmod>2019-06-17</lastmod>
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      <image:title>PhysicsMatt's Blog - Terrible Ideas I've Had</image:title>
      <image:caption>Is this dark matter? I legitimately have no idea. (Daylan et al)</image:caption>
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      <image:title>PhysicsMatt's Blog - Terrible Ideas I've Had</image:title>
      <image:caption>Millisecond Pulsars are so boring. Artists Impression of a Millisecond Pulsar and Binary Companion (Credit: NASA)</image:caption>
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      <image:title>PhysicsMatt's Blog - Terrible Ideas I've Had</image:title>
      <image:caption>pokes Moon with Stick Come ON Moon, do something. Apollo 11, Image Credit: NASA (Also Going-to-the-moon-credit: NASA)</image:caption>
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      <image:title>PhysicsMatt's Blog - Terrible Ideas I've Had</image:title>
      <image:caption>Shown: Not at all what a Interstellar Gas Cloud Looks like Image Credit: Paramount Pictures</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2019/5/13/paper-explainer-direct-detection-anomalies-in-light-of-gaia-data</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2019-05-15</lastmod>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Direct Detection Anomalies in light of Gaia Data</image:title>
      <image:caption>Limits on dark matter elastic spin-independent scattering from XENON1T, CDMSlite, and Cosine-100 assuming the Standard Halo Model, contrasted with the best-fit regions from DAMA/Libra. Fits to the recoil spectrum are shown in orange, and to the daily modulation in yellow.</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Direct Detection Anomalies in light of Gaia Data</image:title>
      <image:caption>Modulation of amount of dark matter capable of causing a dark matter scattering event for the Standard Halo Model (black), the Gaia model for the halo (red), and the S1 stream (blue).</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Direct Detection Anomalies in light of Gaia Data</image:title>
      <image:caption>Limits and Best-fit regions assuming 100% of local dark matter is in the S1 stream and spin-independent Elastic scattering.</image:caption>
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    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1557761562891-AA32Y7K4SMIS65SXRX03/DAMA_Streams_bestfit.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Direct Detection Anomalies in light of Gaia Data</image:title>
      <image:caption>Energy Spectrum of DAMA/Libra observed modulation signal (black), along with S1-only best-fit (Red), and S1+halo best fit (blue).</image:caption>
    </image:image>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1557761670271-1OBARIPYFVXZJYPY198C/DAMA_mass_fraction_bestfit.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Direct Detection Anomalies in light of Gaia Data</image:title>
      <image:caption>Best-fit regions to DAMA/Libra Recoil Spectrum as a function of mass and stream density fraction for spin-independent elastic scatter (yellow, green, orange are 1,2,3 sigma fits). Grey shaded region are parameter points ruled out by null results of other experiments. Note a very small allowed region at 3 sigma near 30 GeV and &gt;80% stream fraction.</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2018/10/16/paper-explainer-asymmetry-observables-and-the-origin-of-rd-anomalies</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2018-10-17</lastmod>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Asymmetry Observables and the Origin of RD^(∗) Anomalies</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Asymmetry Observables and the Origin of RD^(∗) Anomalies</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Asymmetry Observables and the Origin of RD^(∗) Anomalies</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Asymmetry Observables and the Origin of RD^(∗) Anomalies</image:title>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2018/3/14/university-of-oregon-theoretical-physics-seminar</loc>
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    <lastmod>2018-03-14</lastmod>
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      <image:title>PhysicsMatt's Blog - University of Oregon Theoretical Physics Seminar</image:title>
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      <image:caption>Primer on dark matter halos from our paper. The "virial mass" is the mass of the dark matter contained in the halo (and maps to our astrophysical parameter). However, astronomers cannot measure mass directly, and so use proxies like orbital velocities of visible objects (galaxies, stars, and gas) to estimate mass. Presumably the hierarchical structure of halos continues down to ever-smaller scales, but below dwarf galaxies, no visible bodies are known to be embedded in the dark matter halos.</image:caption>
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      <image:caption>A summary of the hints for deviations from predictions of cold dark matter at particular halo mass scales (BTF is "baryonic Tully-Fisher relation" and "TBTF" is "too Big to Fail."), compared to the halo masses where baryonic effects are expected to exist and must be correctly accounted for.</image:caption>
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      <image:caption>Spiral Galaxy NGC 1232 - Credit: ESO</image:caption>
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      <image:caption>Simulated Dark Matter cluster - Credit: Benedikt Diemer, Philip Mansfield</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2017/7/19/paper-explainer-digging-deeper-for-new-physics-in-the-lhc-data</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2017-07-20</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1500515667001-P69B1DP9591MG7BSDR3T/image-asset.png</image:loc>
      <image:title>PhysicsMatt's Blog - Paper Explainer: Digging Deeper for New Physics in the LHC Data</image:title>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Digging Deeper for New Physics in the LHC Data</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Digging Deeper for New Physics in the LHC Data</image:title>
      <image:caption>Global statistical significance as a function of local significance, as estimated from pseudoexperiments using the best-fit model to the anomaly of CMS036 and ATLAS022</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2017/7/13/paper-explainer-collapsed-dark-matter-structures</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2017-07-14</lastmod>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>Pictured: Collapsed Structure built of baryons (Image Credit: NASA)</image:caption>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>PictureD: Collapsed Structure Built of Baryons (Image Credit: NASA)</image:caption>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>Three-Dimensional Map of dark matter constructed by gravitational Lensing Measurements (Image Credit: NASA, ESA and R. Massey (California Institute of Technology)</image:caption>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>Simulation of dark matter. A Milky Way-type galaxy would be located in the center of the yellow blob in the center (Image Credit: MILLENNIUM Simulation)</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>Virgo Cluster of Galaxies (Image Source Rogelio Bernal Andreo via Astronomy Picture of the Day)</image:caption>
    </image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Collapsed Dark Matter Structures</image:title>
      <image:caption>Plot of mass of dark matter halos that can collapse, as function of light dark matter particle mass, assuming heavy dark matter mass of 1.2 TeV. Image from Buckley &amp; DiFranzo 2017.</image:caption>
    </image:image>
  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2017/5/13/paper-explainer-hiding-thermal-dark-matter-with-leptons</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2017-05-14</lastmod>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Hiding Thermal Dark Matter with Leptons</image:title>
      <image:caption>The various ways to look for dark matter, assuming that dark matter is a thermal relic.</image:caption>
    </image:image>
    <image:image>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Hiding Thermal Dark Matter with Leptons</image:title>
      <image:caption>The 1 million parameter points in the leptophilic dark matter model, applying successive experimental tests: a thermal cross section (top), indirect detection (middle), direct detection (bottom). Grey points are excluded, the colored points survive.</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2017/5/4/how-to-show-relativity-must-be-true</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2017-05-05</lastmod>
    <image:image>
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      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>I'm going to construct a thought experiment. It doesn't matter that it's a very unusual situation; all that matters is that it is possible and therefore must be physically consistent.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942553732-F01RUY8NATAMD1RAJ5GE/Blog+-+34.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>1st, let's see how electromagnetism works. Charges create electric fields. Positive charges have fields pointing away from them, negative charges have fields pointing towards.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554174-QGA0KB77XRY6BUG2PD57/Blog+-+35.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Moving charges create magnetic fields. The orientation of those fields "wraps around" the motion of the charge (the fields are "out of the page" here, which is tricky to draw).</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554135-KXFXBSCCM8IG1YHDKCQM/Blog+-+36.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>In the presence of an electric field, a charge feels a force. Positive charges move "with" fields, negative charges move "against."</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554441-4KN05PKTCEWT55GDC3AH/Blog+-+37.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Moving charges in the presence of a magnetic field feel a magnetic force. The force is perpendicular to both the field and the direction of motion (out of the page here).</image:caption>
    </image:image>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554507-6WCWB9RH1CZV4GINASAF/Blog+-+38.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>So, if we have a piece of metal, it is made up of equal numbers of positive and negative charges in a given length of wire. The negative charges move if there is a current, while the positive charges stay stationary.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554789-GJD35NPABB9MXN75HZOP/Blog+-+39.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Since there are equal positive and negative charges, the electrical fields cancel. Since there are moving negative charges and not positive, there is a net magnetic field.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942554895-35CSG8Y5NELT02ARZMXH/Blog+-+40.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>So here's the thought experiment: a positive charge moving next to a wire. We imagine the negative charges in the wire move at the same speed as the positive charge.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555217-804DD5XEWTUMFTDY94B8/Blog+-+41.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>This results in a magnetic force on the charge, and as a result the charge moves away from the wire.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555166-UBLE3WFNBXFAXUD5WAHO/Blog+-+42.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Now, let's imagine what happens if I run alongside the charge at the same speed as it. I'm doing nothing physically to the set up, I'm just changing my frame of reference.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555604-9753C1P1RJ6Q5MNBZCZH/Blog+-+43.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Now I see both the single charge and all the negative charges as stationary, relative to me, and the positive charges in the wire moving backwards.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555603-BMVP1GYTJT9BYMS1L6BQ/Blog+-+44.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>Those moving positive charges create a magnetic field. But since the single charge is now not moving, it feels no magnetic force.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555859-2HHVPOOCES7OFO5KBOS3/Blog+-+45.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>However, we know that the charge must be repelled from the wire. It was in the 1st frame of reference, and I haven't changed the situation at all - just my frame of reference.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942555909-1PK7TEPZJPXHMF681AKS/Blog+-+46.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>So there must be an electric field, point away from the wire. But where could that field come from?</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942556433-FLWXOSV4PLWYXK3YX4WH/Blog+-+47.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>When you eliminate the impossible, whatever remains, however improbable, must be the truth. The electric field must exist, so there must be more positive charges on the wire. Somehow.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942556298-A85UWPVL5FPJ18QFD8ZU/Blog+-+48.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>The answer is relativity. The only way this all works is if length contraction exists. A moving object appears shorter than when it is stationary.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942556520-1E9A1J9UK9MW230MGJC3/Blog+-+49.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>So, the positive charges on the wire were stationary in frame 1. When we run past them, they appear contracted: more positive charges per length.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942556755-OSNWYAISBA4M89N8L18Y/Blog+-+50.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>The negative charges were moving in frame 1. So when we move along with them, they are stationary, and are dilated: fewer charges per length.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942556805-NC63ADMGXP4SOZ9UK710/Blog+-+51.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>So this is what the wire must look like when you run along with the negative charges flowing through it: more positive charges per length than negative.</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/55809d94e4b041b423dad36b/1493942557505-DRMBS3TBSFGT61D4178X/Blog+-+52.png</image:loc>
      <image:title>PhysicsMatt's Blog - How to Show Relativity Must be True</image:title>
      <image:caption>This creates a net electric field, and the positive charge is repelled. This is the only way everyone can see electromagnetism working, regardless of how they are moving through space.</image:caption>
    </image:image>
  </url>
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    <loc>http://www.physicsmatt.com/blog/2017/4/3/conference-talk-theory-overview-of-dark-matter-searches</loc>
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      <image:title>PhysicsMatt's Blog - Conference Talk: Theory Overview of Dark Matter Searches</image:title>
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      <image:title>PhysicsMatt's Blog - Conference Talk: Theory Overview of Dark Matter Searches</image:title>
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      <image:title>PhysicsMatt's Blog - Conference Talk: Theory Overview of Dark Matter Searches</image:title>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2017/1/18/the-twin-paradox-in-special-and-general-relativity</loc>
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    <lastmod>2017-01-27</lastmod>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2016/3/4/paper-explainer-search-for-gamma-ray-emission-from-dark-matter-annihilation-in-the-small-magellanic-cloud-with-the-fermi-large-area-telescope</loc>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope</image:title>
      <image:caption>Artists Rendition of Fermi-LAT (NASA)</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope</image:title>
      <image:caption>Gamma Ray Sky, as Seen by Fermi-LAT (NASA, Fermi Collaboration)</image:caption>
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      <image:caption>Large and Small Magellanic clouds near the Milky Way. Photo from Miloslav Druckmüller</image:caption>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope</image:title>
      <image:caption>Rendition of the Milky way and large and small magellanic clouds. From NASA/CSC/M. Weiss.</image:caption>
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      <image:caption>MAp of the SMC in gamma rays, fermi data. From Caputo et al.</image:caption>
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      <image:caption>Results plot from Caputo et al.</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2016/2/11/ligopalooza</loc>
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    <lastmod>2016-02-11</lastmod>
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      <image:caption>Deflection of light of stars due to the mass of the sun, measured during a solar eclipse (Campbell 1922).</image:caption>
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      <image:caption>LIGO set up (from the LIGO Physical Review Letter). The upper left shows the two locations of the LIGO interferometers in America. The center is a sketch of the interferometer: light is split, sent down the two 4 km arms, and then recombined to see a interference patter. Upper right shows the minimum strain they can measure as a function of frequency.</image:caption>
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      <image:caption>Best fit regions for the mass and total spin of the final black hole after the merger (LIGO)</image:caption>
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      <image:caption>More LIGO data (again from the PRL). The two separate measurements, in the two LIGO locations are shown.</image:caption>
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      <image:caption>LIGO's limit on the wavelength of the graviton, related to the inverse mass of the graviton.</image:caption>
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      <image:caption>Predictions for gravitational wave signals from Cutler and Thorne (gr-qc/0204090)</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2016/1/20/paper-explainer-assessing-astrophysical-uncertainties-in-direct-detection-with-galaxy-simulations</loc>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations</image:title>
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      <image:title>PhysicsMatt's Blog - Paper Explainer: Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations</image:title>
      <image:caption>Map of the Milky Way. Robert Hurt (Spitzer/NASA)</image:caption>
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      <image:caption>Velocity distribution of dark matter in the Galactic reference frame for the four simulated galaxies in  1601.05402. Red is dark matter-only simulations, Blue are simulations with baryons, right column is ratio of baryonic simulation to dark matter.</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2016/1/18/recent-paper-narrow-or-wide-the-phenomenology-of-750-gev-diphotons</loc>
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  <url>
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    <lastmod>2016-03-18</lastmod>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2015/11/20/recent-paper-constraining-the-strength-and-cp-structure-of-dark-production-at-the-lhc-the-associated-top-pair-channel</loc>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Constraining the Strength and CP Structure of Dark Production at the LHC: the Associated Top-Pair Channel</image:title>
      <image:caption>Azimuthal Angle for scalar mediators (black) and pseudoscalar mediators (red) after cut on large transverse momentum. Note the significant difference in angular distribution near 0.</image:caption>
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      <image:caption>Amount of data required to distinguish CP-even and CP-odd mediators with 95% confidence.</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2015/11/20/my-favorite-dark-matter-experiment</loc>
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    <lastmod>2015-11-21</lastmod>
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      <image:caption>Dark matter (called a "WIMP" in this example) scattering with the nuclei of atoms. IMage from University of California, Berkeley</image:caption>
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      <image:caption>Superheated fluid undergoing bubble nucleation. Movie from Juan Collar.</image:caption>
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  </url>
  <url>
    <loc>http://www.physicsmatt.com/blog/2015/10/6/nobelity-neutrino-oscillations</loc>
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    <lastmod>2015-10-08</lastmod>
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      <image:title>PhysicsMatt's Blog - Nobelity: Neutrino Oscillations</image:title>
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      <image:caption>Sketch of neutrino oscillation, from http://www-hep.physics.wm.edu/~vahle/homepage/nuosc.html</image:caption>
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    <image:image>
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      <image:caption>Cherenkov Light in water from the OSU research nuclear reactor.</image:caption>
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    <image:image>
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      <image:caption>Super-Kamiokande (the follow-up experiment to Kamiokande) being filled with water in 1996, with technicians cleaning the photomultiplier detectors</image:caption>
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  <url>
    <loc>http://www.physicsmatt.com/blog/2015/8/4/recent-paper-dark-matter-in-leptophilic-higgs-models-after-the-lhc-run-i</loc>
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      <image:caption>Example Higgs production made possible by Large couplings to top quarks</image:caption>
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    <image:image>
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      <image:caption>Experimental constraints on Higgs parameters in Leptophilic Model.</image:caption>
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      <image:caption>Direct detection constraints for leptophilic Higgs dark matter as parameter $tan\beta$ varied.</image:caption>
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    <loc>http://www.physicsmatt.com/blog/2015/7/25/recent-paper-boosting-the-direct-cp-measurement-of-the-higgs-top-coupling</loc>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
      <image:caption>Top quark-induced interaction between Higgs boson and Gluons</image:caption>
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    <image:image>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
      <image:caption>Example diagram for Higgs-Top production at the LHC.</image:caption>
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    <image:image>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
      <image:caption>Sketch of azimuthal angle, as seen looking down beam axis (direction of proton beam at the LHC).</image:caption>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
      <image:caption>Expected signal strength that can be measured as a function of collected data</image:caption>
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      <image:title>PhysicsMatt's Blog - Recent Paper: Boosting the Direct CP Measurement of the Higgs-Top Coupling</image:title>
      <image:caption>Expected confidence Level at which CP-odd Higgs can be distinguished from CP-even, as a function of collected LHC data.</image:caption>
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  <url>
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    <lastmod>2015-08-01</lastmod>
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      <image:caption>Milky Way Galaxy 21 CM wavelength  (J. Dickey (UMn), F. Lockman (NRAO))</image:caption>
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      <image:caption>Standard Model Particles, via Fermilab</image:caption>
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      <image:caption>Thermal Freeze-Out, JungMan ET AL</image:caption>
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    <lastmod>2016-03-29</lastmod>
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      <image:caption>Spectrum of visible light, relating perceived color with wavelength in nanometers. (Image from Wikipedia)</image:caption>
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      <image:caption>Green Flash at sunset. Image by Brocken Inaglory, via wikipedia.</image:caption>
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      <image:caption>SKetch of the cross sectional area of a sphere of radius r. Red and Blue shaded regions are the cross section looking from the side and top, respectively.</image:caption>
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      <image:caption>Image credit: ESO/L Calçada.</image:caption>
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