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Related papers: Gamma rays from dark mediators in white dwarfs

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Among the several strategies for indirect searches of dark matter, one very promising one is to look for the gamma-rays from decaying dark matter. Here we use the most up-to-date upper bounds on the gamma-ray flux from $10^5$ to $10^{11}$…

High Energy Physics - Phenomenology · Physics 2021-11-17 Marco Chianese , Damiano F. G. Fiorillo , Rasmi Hajjar , Gennaro Miele , Ninetta Saviano

We infer dark matter properties from gamma ray residuals extracted using eight different interstellar emission scenarios proposed by the Fermi-LAT Collaboration to explain the Galactic Center gamma ray excess. Adopting the most plausible…

High Energy Physics - Phenomenology · Physics 2017-03-08 Csaba Balázs , Tong Li

The decay of dark matter particles which are coupled predominantly to charged leptons has been proposed as a possible origin of excess high-energy positrons and electrons observed by cosmic-ray telescopes PAMELA and Fermi LAT. Even though…

High Energy Physics - Phenomenology · Physics 2015-03-17 Mathias Garny , Alejandro Ibarra , David Tran , Christoph Weniger

We propose that the nature of indirect signals of dark matter (DM) can depend on the Galactic environment they originate from. We demonstrate this possibility in models where DM annihilates into light mediators whose branching fractions…

High Energy Physics - Phenomenology · Physics 2023-03-31 Hooman Davoudiasl , Julia Gehrlein

If the dark matter is unstable, the decay of these particles throughout the universe and in the halo of the Milky Way could contribute significantly to the isotropic gamma-ray background (IGRB) as measured by Fermi. In this article, we…

High Energy Astrophysical Phenomena · Physics 2019-03-20 Carlos Blanco , Dan Hooper

Most proposed dark matter candidates are stable and are produced thermally in the early Universe. However, there is also the possibility of unstable (but long-lived) dark matter, produced thermally or otherwise. We propose a strategy to…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-13 Sergio Palomares-Ruiz , Jennifer M. Siegal-Gaskins

Dark matter searches in gamma ray final states often make use of the fact that photons can be produced from final state muons. Modern Monte Carlo generators and DM codes include the effects of final state radiation from muons produced in…

High Energy Physics - Phenomenology · Physics 2016-06-22 Andre Scaffidi , Katherine Freese , Jinmian Li , Christopher Savage , Martin White , Anthony G. Williams

Dark matter (DM) annihilations have been widely studied as a possible explanation of excess gamma rays from the galactic center seen by Fermi/LAT. However most such models are in conflict with constraints from dwarf spheroidals. Motivated…

High Energy Physics - Phenomenology · Physics 2016-07-22 Jeremie Choquette , James M. Cline , Jonathan M. Cornell

Interactions between dark matter (DM) and relativistic particles at early times suppress structure formation on small scales. In particular, the scattering process transfers heat and momentum from radiation to DM, ultimately reducing the…

Cosmology and Nongalactic Astrophysics · Physics 2025-05-14 Wendy Crumrine , Ethan O. Nadler , Rui An , Vera Gluscevic

Dark matter capture and annihilation in the Sun can produce detectable high-energy neutrinos, providing a probe of the dark matter-proton scattering cross section. We consider the case when annihilation proceeds via long-lived dark…

High Energy Astrophysical Phenomena · Physics 2017-07-03 Rebecca K. Leane , Kenny C. Y. Ng , John F. Beacom

Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies between collisionless cold DM and galactic structure observations. However, $\gamma$-ray searches and the CMB strongly constrain such…

High Energy Physics - Phenomenology · Physics 2018-06-27 Iason Baldes , Marco Cirelli , Paolo Panci , Kalliopi Petraki , Filippo Sala , Marco Taoso

We present an improved treatment for the scattering of heavy dark matter from the ion constituents of a white dwarf. In the heavy dark matter regime, multiple collisions are required for the dark matter to become gravitationally captured.…

High Energy Physics - Phenomenology · Physics 2024-07-22 Nicole F. Bell , Giorgio Busoni , Sandra Robles , Michael Virgato

In a medium composed of scalar particles with non-zero mass, the range of Van-der-Waals-type scalar mediated interactions among nucleons becomes infinite when the medium makes a transition to a Bose-Einstein condensed phase. We explore this…

Astrophysics · Physics 2008-11-26 J. A. Grifols

Dark matter particles from the Galactic halo can be gravitationally trapped in the solar core or in external orbits. The enhanced density of dark matter particles either in the solar core or in external orbits can result in the annihilation…

High Energy Astrophysical Phenomena · Physics 2020-07-15 M. N. Mazziotta , F. Loparco , D. Serini , A. Cuoco , P. De La Torre Luque , F. Gargano , M. Gustafsson

We consider the astrophysical bounds on a new form of dark matter, the so called Gravity-mediated Dark Matter. In this scenario, dark matter communicates with us through a mediator sector composed of gravitational resonances, namely a new…

High Energy Physics - Phenomenology · Physics 2015-06-18 Hyun Min Lee , Myeonghun Park , Veronica Sanz

In this paper, we study gamma ray spectra for various scenarios of dark matter annihilation and decay. We focus on processes which generate only high-energy photons or leptons and photons, but no proton-antiproton pairs, to be compatible…

High Energy Physics - Phenomenology · Physics 2009-08-18 Jean-François Fortin , Jessie Shelton , Scott Thomas , Yue Zhao

Using gamma-ray data from observations of the Milky Way, Andromeda (M31), and the cosmic background, we calculate conservative upper limits on the dark matter self-annihilation cross section to a number of final states, over a wide range of…

High Energy Astrophysical Phenomena · Physics 2014-11-20 T. D. Jacques

We consider the search for gamma-rays produced by the annihilation or decay of low-mass dark matter which couples to quarks. In this scenario, most of the photons are produced from the decays of $\pi^0$ or $\eta$ mesons. These decays…

High Energy Physics - Phenomenology · Physics 2023-01-20 J. G. Christy , Jason Kumar , Arvind Rajaraman

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…

High Energy Physics - Phenomenology · Physics 2022-01-19 Cristian Gaidau , Jessie Shelton

Dark matter particles need not be completely stable, and in fact they may be decaying now. We consider this possibility in the frameworks of universal extra dimensions and supersymmetry with very late decays of WIMPs to Kaluza-Klein…

Astrophysics · Physics 2009-06-23 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari