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We analyze the Sun as a source for the indirect detection of dark matter through a search for gamma rays from the solar disk. Capture of dark matter by elastic interactions with the solar nuclei followed by annihilation to long-lived…

高能物理 - 唯象学 · 物理学 2018-12-26 A. Albert , R. Alfaro , C. Alvarez , R. Arceo , J. C. Arteaga-Velázquez , D. Avila Rojas , H. A. Ayala Solares , E. Belmont-Moreno , S. Y. BenZvi , C. Brisbois , K. S. Caballero-Mora , T. Capistràn , A. Carramiñana , S. Casanova , M. Castillo , J. Cotzomi , S. Coutiño de León , C. De León , E. De la Fuente , S. Dichiara , B. L. Dingus , M. A. DuVernois , J. C. Díaz-Vélez , K. Engel , O. Enríquez-Rivera , C. Espinoza , H. Fleischhack , N. Fraija , J. A. García-González , F. Garfias , M. M. González , J. A. Goodman , Z. Hampel-Arias , J. P. Harding , S. Hernandez , B. Hona , F. Hueyotl-Zahuantitla , P. Hüntemeyer , A. Iriarte , A. Jardin-Blicq , V. Joshi , S. Kaufmann , H. León Vargas , G. Luis-Raya , J. Lundeen , R. López-Coto , K. Malone , S. S. Marinelli , O. Martinez , I. Martinez-Castellanos , J. Martínez-Castro , P. Miranda-Romagnoli , E. Moreno , M. Mostafá , A. Nayerhoda , L. Nellen , M. Newbold , M. U. Nisa , R. Noriega-Papaqui , J. Pretz , E. G. Pérez-Pérez , Z. Ren , C. D. Rho , C. Rivière , D. Rosa-González , M. Rosenberg , E. Ruiz-Velasco , H. Salazar , F. Salesa Greus , A. Sandoval , M. Schneider , M. Seglar Arroyo , G. Sinnis , A. J. Smith , P. Surajbali , I. Taboada , O. Tibolla , K. Tollefson , I. Torres , L. Villaseñor , T. Weisgarber , S. Westerhoff , I. G. Wisher , J. Wood , T. Yapici , A. Zepeda , H. Zhou , J. D. Álvarez , J. F. Beacom , R. K. Leane , T. Linden , K. C. Y. Ng , A. H. G. Peter , B. Zhou

We calculate the scattering rate of sub-GeV dark matter in solid-state targets for spin-dependent dark matter -- nucleon interactions. For dark matter particles with mass below 100 MeV, the scattering occurs predominantly through incoherent…

高能物理 - 唯象学 · 物理学 2025-06-16 Stefania Gori , Simon Knapen , Tongyan Lin , Pankaj Munbodh , Bethany Suter

We analyze the direct detection signals of a toy model consisting of a Dirac dark matter particle which couples to one Standard Model fermion via a scalar mediator. For all scenarios, the dark matter particle scatters off nucleons via one…

高能物理 - 唯象学 · 物理学 2015-06-03 Alejandro Ibarra , Sebastian Wild

So far, the observed effects of dark matter are compatible with it having purely gravitational interactions. However, in many models, dark matter has additional interactions with itself, with the Standard Model, and/or with additional…

高能物理 - 唯象学 · 物理学 2021-01-21 Robert Lasenby

We point out a new and largely model-independent constraint on the dark matter scattering cross section with nucleons, applying when this quantity is larger than for typical weakly interacting dark matter candidates. When the dark matter…

天体物理学 · 物理学 2008-11-26 Gregory D. Mack , John F. Beacom , Gianfranco Bertone

We propose a new strategy to directly detect light particle dark matter that has long-ranged interactions with ordinary matter. The approach involves distorting the local flow of dark matter with time-varying fields and measuring these…

高能物理 - 唯象学 · 物理学 2020-01-08 Asher Berlin , Raffaele Tito D'Agnolo , Sebastian A. R. Ellis , Philip Schuster , Natalia Toro

We study self-interacting dark matter coupled to the Standard Model via the Higgs portal. We consider a scenario where dark matter is a thermal relic with strong enough self interactions that can alleviate the problems of collisionless cold…

高能物理 - 唯象学 · 物理学 2015-03-05 Chris Kouvaris , Ian M. Shoemaker , Kimmo Tuominen

Recent high-quality observations of dwarf and low surface brightness (LSB) galaxies have shown that their dark matter (DM) halos prefer flat central density profiles. On the other hand the standard cold dark matter model simulations predict…

星系天体物理 · 物理学 2021-02-17 T. Matos , Victor H. Robles

Brown dwarfs, being transitional objects between giant planets and low-mass stars, possess dense, cool interiors that provide optimal conditions to explore non-standard physics. Capture and accumulation of dark-matter particles can alter…

太阳与恒星天体物理 · 物理学 2026-05-15 A. Pérez-Garrido

Dark matter that is capable of sufficiently heating a local region in a white dwarf will trigger runaway fusion and ignite a type Ia supernova. This was originally proposed in Graham et al. (2015) and used to constrain primordial black…

高能物理 - 唯象学 · 物理学 2019-01-02 Peter Graham , Ryan Janish , Vijay Narayan , Surjeet Rajendran , Paul Riggins

Many models containing particles which are candidates for dark matter, assume the standard model particles and the dark matter candidates are mediated by a spin-0 particle. At the LHC, one can use these models for dark matter searches. One…

高能物理 - 实验 · 物理学 2019-03-20 Yoav Afik , Eitan Gozani , Yoram Rozen

Light dark matter (DM) with mass around the GeV scale faces weaker bounds from direct detection experiments. If DM couples strongly to a light mediator, it is possible to have observable direct detection rate. However, this also leads to a…

高能物理 - 唯象学 · 物理学 2024-11-21 Amit Adhikary , Debasish Borah , Satyabrata Mahapatra , Indrajit Saha , Narendra Sahu , Vicky Singh Thounaojam

We present a model of vector dark matter that interacts through a low-mass vector mediator based on the Higgsing of an SU(2) dark sector. The dark matter is charged under a U(1) gauge symmetry. Even though this symmetry is broken, the…

高能物理 - 唯象学 · 物理学 2020-04-08 Ian Chaffey , Philip Tanedo

We re-examine the gravitational capture of dark matter (DM) through long-range interactions. We demonstrate that neglecting the thermal motion of target particles, which is often a good approximation for short-range capture, results in…

高能物理 - 唯象学 · 物理学 2022-01-19 Cristian Gaidau , Jessie Shelton

Mass estimates of white dwarfs via electromagnetic methods, often differ from those obtained through gravitational redshift measurements, in some cases with discrepancies ranging in $5-15\%$ across independent datasets. Although many of the…

高能天体物理现象 · 物理学 2025-11-04 Jorge Castelo Mourelle , Nicolas Sanchis-Gual , José A. Font , Juan Calderón Bustillo

Dark matter could have a dissipative asymmetric subcomponent in the form of atomic dark matter (aDM). This arises in many scenarios of dark complexity, and is a prediction of neutral naturalness, such as the Mirror Twin Higgs model. We show…

高能物理 - 唯象学 · 物理学 2021-06-25 David Curtin , Jack Setford

Direct detection of dark matter (DM) requires an interaction of dark matter particles with nucleons. The same interaction can lead to dark matter pair production at a hadron collider, and with the addition of initial state radiation this…

高能物理 - 唯象学 · 物理学 2011-01-05 Yang Bai , Patrick J. Fox , Roni Harnik

A search for dark matter is conducted in final states containing a photon and missing transverse momentum in proton$-$proton collisions at $\sqrt{s}$ = 13 TeV. The data, collected during 2015$-$2018 by the ATLAS experiment at the CERN LHC,…

高能物理 - 实验 · 物理学 2021-04-14 ATLAS Collaboration

We study the interaction of an electrically charged component of the dark matter with a magnetized galactic interstellar medium (ISM) of (rotating) spiral galaxies. For the observed ordered component of the field, $B\sim \mu$G, we find that…

宇宙学与河外天体物理 · 物理学 2019-12-04 Albert Stebbins , Gordan Krnjaic

We analyze strongly lensed images in 8 galaxy clusters to measure their dark matter density profiles in the radial region between 10 kpc and 150 kpc, and use this to constrain the self-interaction cross section of dark matter (DM)…

宇宙学与河外天体物理 · 物理学 2021-11-24 Kevin E. Andrade , Jackson Fuson , Sophia Gad-Nasr , Demao Kong , Quinn Minor , M. Grant Roberts , Manoj Kaplinghat