text:   darkmatter annihilation in FIRE simulations",6,"['New paper led by @UCIPhysAstro PhD student @danphysic uses FIRE simulations to predict J-factors for DM-indirect detection @ Galactic Center ➡️Velocity-dependent p &amp; d-wave annihilation amplified compared to dark-matter-only expectations @UCIrvineGD <LINK> <LINK>', ""For p-wave annihilation ~(v/c)^2, standard expectation is these models not detectable because v&lt;&lt;c in Milky Way.  We find signal is ~10 times higher than you'd expect from dark-matter-only =&gt; p-wave models w/ correct thermal abundance may be within the range of detection! https://t.co/QAT5V6A4jF"", 'The reason for enhancement is that dark-matter particle velocities are significantly enhanced in the Galactic Center compared to dark-matter-only simulations - a result of galaxy formation https://t.co/cjtJ9xRyDs', 'What fantastic work by Daniel McKeown @danphysic and wonderful collaborators @AstronoMerc_ @ZachHafen @MBKplus @AndrewWetzel @linoush95  @PFHopkins_Astro @AstroBananna - Congratulations! https://t.co/IzgRLdyiwO', '@TillSawala @UCIPhysAstro @danphysic @UCIrvineGD For p &amp; d-wave, yes. Dwarfs harder. Clusters easier though.', '@ProfTimTait @danphysic @AstronoMerc_ @ZachHafen @MBKplus @AndrewWetzel @linoush95 @PFHopkins_Astro @AstroBananna Yes!  Simona was on @danphysic advancement so has a heads up!']",21,11,1224