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The Standard Model of particle physics can be extended to include sterile (right-handed) neutrinos or axions to solve the dark matter problem. Depending upon the mixing angle between active and sterile neutrinos, the latter have the…

High Energy Astrophysical Phenomena · Physics 2017-06-28 A. Gewering-Peine , D. Horns , J. H. M. M. Schmitt

Numerous astrophysical and cosmological observations are best explained by the existence of dark matter, a mass density which interacts only very weakly with visible, baryonic matter. Searching for the extremely weak signals produced by…

Large-volume neutrino experiments are ideal for testing boosted dark matter (BDM) scenarios. We propose, for the first time, an approach to utilize knockout neutrons by detecting de-excitation $\gamma$ rays and coincident captured neutrons…

High Energy Physics - Phenomenology · Physics 2024-09-10 Koun Choi , Jong-Chul Park

Direct detection of light dark matter can be significantly enhanced by up-scattering of dark matter with energetic particles in the cosmic ambient. This boosted dark matter flux can reach kinetic energies up to tens of MeV, while the…

High Energy Physics - Phenomenology · Physics 2025-03-18 Dilip Kumar Ghosh , Tushar Gupta , Matti Heikinheimo , Katri Huitu , Sk Jeesun

We propose a cosmological scenario based on the assumption that the Standard Model possesses a large number of copies. It is demonstrated that baryons in the hidden copies of the standard model can naturally account for the dark matter. The…

High Energy Physics - Theory · Physics 2009-08-11 Gia Dvali , Ignacy Sawicki , Alexander Vikman

Dark Matter constitutes most of the matter in the presently accepted cosmological model for our Universe. The extreme conditions of ordinary baryonic matter, namely high density and compactness, in Neutron Stars make these objects suitable…

High Energy Astrophysical Phenomena · Physics 2017-10-20 M. Cermeño , M. Ángeles Pérez-García , Joseph Silk

The dark-matter candidates of particle physics invariably possess electromagnetic interactions, if only via quantum fluctuations. Taken en masse, dark matter can thus engender an index of refraction which deviates from its vacuum value. Its…

High Energy Physics - Phenomenology · Physics 2014-11-18 S. Gardner , D. C. Latimer

To constrain the properties of dark matter (DM) that interacts with nucleons, we have conducted an experimental search for any anomalous heating of ordinary baryonic matter at 77 K. Our tabletop experiment is motivated by the possibility…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-29 David A. Neufeld , Daniel J. Brach-Neufeld

We study a new dark sector signature for an atomic process of "rearrangement" in the galaxy. In this process, a hydrogen-like atomic dark matter state together with its anti-particle can rearrange to form a highly-excited bound state. This…

High Energy Physics - Phenomenology · Physics 2021-04-21 James Eiger , Michael Geller

Why matter and dark matter contents of the universe are of the same order of magnitude, is one of the puzzles of modern cosmology. At the face of it, this would seem to point towards a basic similarity between matter and dark matter,…

High Energy Physics - Phenomenology · Physics 2025-02-24 Rabindra N. Mohapatra , Nobuchika Okada

The identification of the nature of dark matter is one of the most important problems confronting particle physics. Current observational constraints permit the mass of the dark matter to range from $10^{-22}$ eV - $10^{48}$ GeV. Given the…

High Energy Physics - Phenomenology · Physics 2022-04-08 Surjeet Rajendran

Dark matter is a fundamental constituent of the universe, which is needed to explain a wide variety of astrophysical and cosmological observations. Although the existence of dark matter was first postulated nearly a century ago and its…

Cosmology and Nongalactic Astrophysics · Physics 2025-09-23 Csaba Balazs , Torsten Bringmann , Felix Kahlhoefer , Martin White

Ultralight dark photons are compelling dark matter candidates, but their allowed kinetic mixing with the Standard Model photon is severely constrained by requiring that the dark photons do not collapse into a cosmic string network in the…

High Energy Physics - Phenomenology · Physics 2025-08-20 David Cyncynates , Zachary J. Weiner

An appealing candidate of the galactic dark matter is the axion, which was postulated to solve the strong CP (Charge-conjugation Parity) violation problem in the standard particle theory. A new experimental method is proposed to determine…

High Energy Physics - Phenomenology · Physics 2018-06-18 M. Yoshimura , N. Sasao

We propose here a set of new methods to directly detect light mass dark matter through its scattering with abundant atmospheric muons or accelerator beams. Firstly, we plan to use the free cosmic-ray muons interacting with dark matter in a…

The search for dark matter and physics beyond the Standard Model has grown to encompass a highly interdisciplinary approach. In this review, we survey recent searches for light, weakly-coupled particles - axions and dark photons - over the…

High Energy Physics - Phenomenology · Physics 2024-12-13 Asher Berlin , Yonatan Kahn

We present a novel mechanism of using solar neutrinos to speed up dark matter, inspired by the fact that neutrinos are the most energetic particles from the Sun with a well-understood spectrum. In a neutrino portal dark sector model, we…

High Energy Physics - Phenomenology · Physics 2022-01-25 Yue Zhang

Dark photon is a massive vector particle which couples to the physical photon through the kinetic mixing term. Such particles, if exist, are produced in photon beams and, in particular, in laser radiation. Due to the oscillations between…

High Energy Physics - Phenomenology · Physics 2019-06-19 V. V. Flambaum , I. B. Samsonov , H. B. Tran Tan

We investigate the physics of dark matter models featuring composite bound states carrying a large conserved dark "nucleon" number. The properties of sufficiently large dark nuclei may obey simple scaling laws, and we find that this scaling…

High Energy Physics - Phenomenology · Physics 2021-01-21 Edward Hardy , Robert Lasenby , John March-Russell , Stephen M. West

We argue that Dark Matter can be described by an interacting field theory with a mass parameter of the order of the proton mass and an interaction coupling of the order of the QED coupling.

General Relativity and Quantum Cosmology · Physics 2008-11-26 Elcio Abdalla , Bin Wang
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