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Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Christian G. Boehmer , Gabriela Caldera-Cabral , Ruth Lazkoz , Roy Maartens

Dark matter (DM) is a new type of invisible matter introduced to explain various features of recent astrophysical observations, including galaxy rotation curves and other fundamental characteristics of our universe. DM may couple to…

High Energy Physics - Experiment · Physics 2025-06-24 Vindhyawasini Prasad

Recently there has been much interest in hidden sectors, especially in the context of dark matter and dark forces, since they are a common feature of beyond standard model scenarios like string theory and SUSY and additionally exhibit…

High Energy Physics - Phenomenology · Physics 2012-11-26 Sarah Andreas

A number of proposed and ongoing experiments search for axion dark matter with a mass nearing the limit set by small scale structure (${\cal O} ( 10 ^{ - 21 } {\rm eV} ) $). We consider the late universe cosmology of these models, showing…

High Energy Physics - Phenomenology · Physics 2021-01-11 Jeff A. Dror , Jacob M. Leedom

X-ray telescopes are an exceptional tool for searching for new fundamental physics. In particular, X-ray observations have already placed world-leading bounds on the interaction between photons and axion-like particles (ALPs). ALPs are…

High Energy Physics - Phenomenology · Physics 2018-04-11 Francesca Day , Sven Krippendorf

If there are a plethora of axions in nature, they may have a complicated potential and create an axion landscape. We study a possibility that one of the axions is so light that it is cosmologically stable, explaining the observed dark…

High Energy Physics - Phenomenology · Physics 2017-03-03 Ryuji Daido , Takeshi Kobayashi , Fuminobu Takahashi

Solutions to the hierarchy problem that require partners for each standard model particle often require that these states live at or above the electroweak scale, to satisfy phenomenological bounds. Partners to possible dark sector particles…

High Energy Physics - Phenomenology · Physics 2015-06-18 Christopher D. Carone

Modern astronomical data on galaxy and cosmological scales have revealed powerfully the existence of certain dark sectors of fundamental physics, i.e., existence of particles and fields outside the standard models and inaccessible by…

Astrophysics · Physics 2008-12-18 HongSheng Zhao

We review dark matter (DM) candidates of a very low mass, appearing in the window below the traditional weakly-interacting massive particle $m_\chi \lesssim 10$ GeV and extending down to $m_\chi \gtrsim 1$ meV, somewhat below the mass limit…

High Energy Physics - Phenomenology · Physics 2025-02-25 Kathryn M. Zurek

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling between dark energy and dark matter. However, the signature of the coupling is not easy to grasp, since the coupling is degenerate…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-22 Jian-Hua He , Bin Wang , Elcio Abdalla

Axions and axion like particles are very attractive dark matter candidates. In this review, we briefly investigate how the cosmological observations reveal the existence of dark matter and some unique properties of axions/axion like…

High Energy Physics - Phenomenology · Physics 2017-04-12 Qiaoli Yang

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

High Energy Physics - Phenomenology · Physics 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

We review the motivation for the axion as a solution of the strong CP puzzle and as a candidate for cold dark matter. Then we discuss benchmark axion models and present their predictions concerning axion couplings to the Standard Model and…

High Energy Physics - Phenomenology · Physics 2023-11-21 Andreas Ringwald

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and mechanisms of its symmetry breaking. Particle candidates for cosmological dark matter are…

Cosmology and Nongalactic Astrophysics · Physics 2013-11-12 Maxim Yu. Khlopov

For physicists, recent developments in astrophysics and cosmology present exciting challenges. We are conducting "experiments" in energy regimes some of which will be probed by accelerators in the near future, and others which are…

High Energy Physics - Theory · Physics 2007-05-23 Michael Dine

We argue that the striking similarity between the cosmic abundances of baryons and dark matter, despite their very different astrophysical behavior, strongly motivates the scenario in which dark matter resides within a rich dark sector…

High Energy Physics - Phenomenology · Physics 2024-06-13 Arushi Bodas , Manuel A. Buen-Abad , Anson Hook , Raman Sundrum

We investigate the constraints of dark matter search experiments on the different candidates emerging from the minimal quasi-conformal strong coupling theory with fermions in the adjoint representation. For one candidate, the current limits…

High Energy Physics - Phenomenology · Physics 2010-04-30 Chris Kouvaris

We review the physical and cosmological consequences of two possible electromagnetic couplings to the dark sector: (i) a neutral lightest dark-matter particle (LDP) with nonzero electric and/or magnetic dipole moments and (ii) a charged…

Astrophysics · Physics 2007-05-23 Kris Sigurdson

The existence of dark matter particles that carry phenomenologically relevant self-interaction cross sections mediated by light dark sector states is considered to be severely constrained through a combination of experimental and…

High Energy Physics - Phenomenology · Physics 2020-04-08 Nicolás Bernal , Xiaoyong Chu , Suchita Kulkarni , Josef Pradler
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