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Superheavy dark matter has been attractive as a candidate of particle dark matter. We propose a ``natural" particle model, in which the dark matter serves as the inflaton in natural inflation, while decaying to high-energy particles at…

High Energy Physics - Phenomenology · Physics 2025-12-03 Kohta Murase , Yuma Narita , Wen Yin

We analyze the effect of Dark Matter (DM) - Standard Model (SM) non-gravitational interactions on the orbital dynamics of celestial bodies near the supermassive black hole Sagittarius A*, where the DM density is generically expected to be…

High Energy Physics - Phenomenology · Physics 2025-10-03 Javier F. Acevedo , Aidan J. Reilly , Lillian Santos-Olmsted

Neutron stars can provide new insight into dark matter properties, as these dense objects capture dark matter particles very efficiently. It has recently been shown that the energy transfer in the dark matter capture process can lead to…

High Energy Physics - Phenomenology · Physics 2018-09-13 Nicole F. Bell , Giorgio Busoni , Sandra Robles

We examine a simple dark sector extension where the observed dark matter (DM) abundance arises from a freeze-in process through the decay of heavy vector-like quarks into a scalar dark matter candidate. The detection prospects of such DM…

High Energy Physics - Phenomenology · Physics 2025-09-23 Anupam Ghosh , Partha Konar , Sudipta Show

The explorations of alternative dark matter (DM) candidates beyond WIMP motivated primordial black holes (PBHs) or sub-GeV DM particle in the Milky Way. Neutrinos from PBH evaporation at the present times play as a novel medium boosting…

High Energy Physics - Phenomenology · Physics 2021-08-13 Wei Chao , Tong Li , Jiajun Liao

Dark matter particles will be captured in neutron stars if they undergo scattering interactions with nucleons or leptons. These collisions transfer the dark matter kinetic energy to the star, resulting in appreciable heating that is…

High Energy Physics - Phenomenology · Physics 2019-07-02 Nicole F. Bell , Giorgio Busoni , Sandra Robles

Direct detection experiments have started to explore dark matter scattering off electrons and nucleons through light mediators. Mediators with sub-keV masses are efficiently produced in the Sun and can be absorbed in the same detectors that…

High Energy Physics - Phenomenology · Physics 2026-02-27 Pieter Braat , Anh Vu Phan , Marieke Postma , Susanne Westhoff

For dark matter to be detectable with gravitational waves from binary black holes, it must reach higher than average densities in their vicinity. In the case of light (wave-like) dark matter, the density of dark matter between the binary…

General Relativity and Quantum Cosmology · Physics 2024-05-29 Josu C. Aurrekoetxea , Katy Clough , Jamie Bamber , Pedro G. Ferreira

Assuming that (1) the universe underwent a post-inflationary accelerated expansion phase driven by a fluid with equation of state $P=w\rho$ and $-1<w<-1/3$, that (2) the cosmic horizon in an accelerating, quasi-de Sitter universe has a…

High Energy Physics - Phenomenology · Physics 2025-06-24 Stefano Profumo

We point out a new type of diurnal effect for the cosmic ray boosted dark matter (DM). The DM-nucleon interactions not only allow the direct detection of DM with nuclear recoils, but also allow cosmic rays to scatter with and boost the…

High Energy Physics - Phenomenology · Physics 2021-03-17 Shao-Feng Ge , Jiang-Lai Liu , Qiang Yuan , Ning Zhou

The observed dark matter abundance in the Universe can be fully accounted for by a minimally coupled spectator scalar field that was light during inflation and has sufficiently strong self-coupling. In this scenario, dark matter was…

Cosmology and Nongalactic Astrophysics · Physics 2019-01-03 Tommi Markkanen , Arttu Rajantie , Tommi Tenkanen

We report detailed studies of the X-ray emission from the kpc scale jet in the nearest active galaxy, Cen A. 41 compact sources were found within the jet, 13 of which were newly identified. We construct the luminosity function for the…

Cosmic rays scattering with neutrinos produced in supernovae induce a flux of supernova neutrinos boosted to high energies. We calculate the neutrino flux arising from this new mechanism in environments with large cosmic-ray and supernova…

High Energy Physics - Phenomenology · Physics 2025-08-19 Gonzalo Herrera , Shunsaku Horiuchi

Dark stars (DSs) -- first stars powered by dark-matter (DM) heating rather than fusion -- could form in the early Universe. They can grow to $\gtrsim 10^5 M_{\odot}$ masses and collapse into seeds of supermassive black holes (SMBHs). We…

High Energy Physics - Phenomenology · Physics 2025-05-23 Thomas Schwemberger , Volodymyr Takhistov

A novel analysis is performed, incorporating time-of-flight (TOF) information to study the interactions of dark matter (DM) with standard model particles. After supernova (SN) explosions, DM with mass $m_\chi\lesssim\mathcal{O}({\rm MeV})$…

High Energy Physics - Phenomenology · Physics 2024-05-03 Yen-Hsun Lin , Wen-Hua Wu , Meng-Ru Wu , Henry Tsz-King Wong

Dark photon is a new gauge boson beyond the Standard Model as a kind of dark matter (DM) candidate. Dark photon dark matter (DPDM) interacts with electromagnetic fields via kinetic mixing, implicating an approach to give a constraint with…

High Energy Astrophysical Phenomena · Physics 2024-07-24 Tian-Ci Liu , Ming-Xuan Lu , Xiao-Song Hu

Recently, one of the present authors noticed a stimulated emission process of bosonic dark matter via the two-body decay of a mother particle in a thermal plasma similar to the operation principle of a laser in 2301.08735. In this paper, we…

High Energy Physics - Phenomenology · Physics 2024-10-25 Kodai Sakurai , Wen Yin

We perform full 3D numerical simulations of compact objects, such as black holes or neutron stars, boosted through an ambient force-free plasma that posses a uniform magnetization. We study jet formation and energy extraction from the…

High Energy Astrophysical Phenomena · Physics 2019-09-25 Ramiro Cayuso , Federico Carrasco , Barbara Sbarato , Oscar Reula

We demonstrate how the two dominant constituents of the Universe, dark energy and dark matter, could possess a large scattering cross-section without considerably impacting observations. Unlike models involving energy exchange between the…

Cosmology and Nongalactic Astrophysics · Physics 2010-10-27 Fergus Simpson
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