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Cold dark matter (CDM) models predict small-scale structure in excess of observations of the cores and abundance of dwarf galaxies. These problems might be solved, and the virtues of CDM models retained, even without postulating {\it ad…

Astrophysics · Physics 2009-10-31 Wayne Hu , Rennan Barkana , Andrei Gruzinov

There have been proposals that primordial black hole remnants (BHRs) are the dark matter, but the idea is somewhat vague. We argue here first that the generalized uncertainty principle (GUP) may prevent black holes from evaporating…

Astrophysics · Physics 2017-08-23 Pisin Chen

We consider galaxy halos formed by dark matter bosons with mass in the range of about a few tens or hundreds eV. A major part of the particles is in a noncondensed state and described under the Thomas-Fermi approach. Derived equations are…

Astrophysics of Galaxies · Physics 2021-12-08 Iskander G. Abdullin , Vladimir A. Popov

We assume dark matter to be a cosmological self-gravitating Bose-Einstein condensate of non-relativistic ultralight scalar particles with competing gravitational and repulsive contact interactions and investigate the observational…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-19 V. Delgado , A. Muñoz Mateo

We propose that dark matter consists of collections of atoms encapsulated inside pieces of an alternative vacuum, in which the Higgs field vacuum expectation value is appreciably smaller than in the usual vacuum. The alternative vacuum is…

Astrophysics · Physics 2007-05-23 C. D. Froggatt , H. B. Nielsen

Dark matter is postulated as a light fermion in two natural scenarios as the outcome of a softly broken discrete symmetry. It is produced from the naturally suppressed decay of the standard-model Higgs boson through the freeze-in mechanism.

High Energy Physics - Phenomenology · Physics 2024-09-25 Ernest Ma

Dark Matter is one of the most intriguing riddles of modern astrophysics. The Standard Cosmological Model implies that only 4.5% of the mass-energy of the Universe is baryonic matter and the remaining 95% is unknown. Of this remainder, 22%…

Instrumentation and Methods for Astrophysics · Physics 2010-11-19 Andrzej M. Szelc

This short review was prepared as an introduction to the Royal Society's 'Dark Matter' conference. It addresses the embarrassing fact that 95% of the universe is unaccounted for. Favoured dark matter candidates are axions or…

Astrophysics · Physics 2010-12-09 Martin J. Rees

One of the leading candidates for dark matter is axion or axion-like particle in a form of Bose-Einstein condensate (BEC). In this paper, we present an analysis of 17 high-resolution galactic rotation curves from "The H{\footnotesize I}…

Astrophysics of Galaxies · Physics 2014-08-04 Ming-Hua Li , Zhi-Bing Li

The identity of dark matter is a question of central importance in both astrophysics and particle physics. In the past, the leading particle candidates were cold and collisionless, and typically predicted missing energy signals at particle…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-03 Jonathan L. Feng

Mirror matter is a stable self-collisional dark matter candidate. If parity is a conserved unbroken symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe composed of particles with the same masses and…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-31 Paolo Ciarcelluti

The main aim of this study is to reveal curved space and particle physics effects on the formation of Bose-Einstein condensate (BEC) scalar fields in cosmology and around a black hole. Cosmological scalar fields for dark energy and dark…

General Relativity and Quantum Cosmology · Physics 2023-08-11 Kemal Gültekin

We develop our novel model of cosmology based on the Bose-Einstein condensation. This model unifies the Dark Energy and the Dark Matter, and predicts multiple collapse of condensation, followed by the final acceleration regime of cosmic…

Astrophysics · Physics 2009-06-23 Takeshi Fukuyama , Masahiro Morikawa , Takayuki Tatekawa

Cosmological and astrophysical measurements indicate that the universe contains a large amount of dark matter. A number of weak scale dark matter candidates have been proposed in extensions of the standard model. The potential to discover…

High Energy Physics - Phenomenology · Physics 2009-12-17 G. Bélanger

The dark sector of the Universe is beginning to be clarified step by step. If the dark energy is vacuum energy, then 123 orders are exactly reduced by ordinary physical processes. For many years these unexplained orders were called a crisis…

General Physics · Physics 2017-05-31 Vladimir Burdyuzha

Mirror matter is a stable self-collisional dark matter candidate. If exact mirror parity is a conserved symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Paolo Ciarcelluti

The axion, which has yet to be discovered, is a promising candidate for dark matter that emerges from Peccei-Quinn theory. This article presents the search for axion dark matter with the "Student Project for an Axion Cavity Experiment"…

High Energy Physics - Experiment · Physics 2025-10-29 M. A. Akgümüs , N. Salama , J. Egge , E. Garutti , M. Maroudas , L. H. Nguyen , D. Leppla-Weber

We propose a mechanism for origin of matter in the universe in the framework of Einstein-Gauss-Bonnet gravity in higher dimensions. The recently discovered new static black hole solution by the authors \cite{md2006} with the Kaluza-Klein…

High Energy Physics - Theory · Physics 2008-11-26 Naresh Dadhich , Hideki Maeda

Historically the most popular dark matter candidates have been new elementary particles, such as Weakly Interacting Massive Particles and axions. However Primordial Black Holes (PBHs), black holes formed from overdensities in the early…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-26 Anne M. Green

The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. Transformative advances in quantum technologies have led to a plethora of new…

High Energy Physics - Experiment · Physics 2022-03-29 D. Antypas , A. Banerjee , C. Bartram , M. Baryakhtar , J. Betz , J. J. Bollinger , C. Boutan , D. Bowring , D. Budker , D. Carney , G. Carosi , S. Chaudhuri , S. Cheong , A. Chou , M. D. Chowdhury , R. T. Co , J. R. Crespo López-Urrutia , M. Demarteau , N. DePorzio , A. V. Derbin , T. Deshpande , M. D. Chowdhury , L. Di Luzio , A. Diaz-Morcillo , J. M. Doyle , A. Drlica-Wagner , A. Droster , N. Du , B. Döbrich , J. Eby , R. Essig , G. S. Farren , N. L. Figueroa , J. T. Fry , S. Gardner , A. A. Geraci , A. Ghalsasi , S. Ghosh , M. Giannotti , B. Gimeno , S. M. Griffin , D. Grin , D. Grin , H. Grote , J. H. Gundlach , M. Guzzetti , D. Hanneke , R. Harnik , R. Henning , V. Irsic , H. Jackson , D. F. Jackson Kimball , J. Jaeckel , M. Kagan , D. Kedar , R. Khatiwada , S. Knirck , S. Kolkowitz , T. Kovachy , S. E. Kuenstner , Z. Lasner , A. F. Leder , R. Lehnert , D. R. Leibrandt , E. Lentz , S. M. Lewis , Z. Liu , J. Manley , R. H. Maruyama , A. J. Millar , V. N. Muratova , N. Musoke , S. Nagaitsev , O. Noroozian , C. A. J. O'Hare , J. L. Ouellet , K. M. W. Pappas , E. Peik , G. Perez , A. Phipps , N. M. Rapidis , J. M. Robinson , V. H. Robles , K. K. Rogers , J. Rudolph , G. Rybka , M. Safdari , M. Safdari , M. S. Safronova , C. P. Salemi , P. O. Schmidt , T. Schumm , A. Schwartzman , J. Shu , M. Simanovskaia , J. Singh , S. Singh , M. S. Smith , W. M. Snow , Y. V. Stadnik , C. Sun , A. O. Sushkov , T. M. P. Tait , V. Takhistov , D. B. Tanner , D. J. Temples , P. G. Thirolf , J. H. Thomas , M. E. Tobar , O. Tretiak , Y. -D. Tsai , J. A. Tyson , M. Vandegar , S. Vermeulen , L. Visinelli , E. Vitagliano , Z. Wang , D. J. Wilson , L. Winslow , S. Withington , M. Wooten , J. Yang , J. Ye , B. A. Young , F. Yu , M. H. Zaheer , T. Zelevinsky , Y. Zhao , K. Zhou