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We present a simple UV completion of Atomic Dark Matter (aDM) in which heavy right-handed neutrinos decay to induce both dark and lepton number densities. This model addresses several outstanding cosmological problems: the…

高能物理 - 唯象学 · 物理学 2015-05-28 David E. Kaplan , Gordan Z. Krnjaic , Keith R. Rehermann , Christopher M. Wells

Gravitinos with a mass in the keV range are an interesting candidate for warm dark matter. Recent measurements of the matter density of the universe and of cosmic structures at the dwarf galaxy scale rule out the simplest gravitino models…

天体物理学 · 物理学 2009-11-07 Edward A. Baltz , Hitoshi Murayama

We discuss variants of Cold Dark Matter (CDM) dominated cosmological models that give good agreement with a range of observations. We consider models with hot dark matter, tilt, $\Omega < 1$, or a cosmological constant. We also discuss the…

天体物理学 · 物理学 2007-05-23 Rachel S. Somerville , Joel R. Primack

Ultralight axions which couple sufficiently strongly to photons can leave imprints on the sky at diverse frequencies by mixing with cosmic light in the presence of background magnetic fields. We explore such direction dependent grey-body…

宇宙学与河外天体物理 · 物理学 2015-04-16 Guido D'Amico , Nemanja Kaloper

The axino is a promising candidate for dark matter in the Universe. It is electrically and color neutral, very weakly interacting, and could be - as assumed in this study - the lightest supersymmetric particle, which is stable for unbroken…

高能物理 - 唯象学 · 物理学 2009-11-10 Arnd Brandenburg , Frank Daniel Steffen

After a period of inflationary expansion, the Universe reheated and reached full thermal equilibrium at the reheating temperature T_R. In this work we point out that, in the context of effective low-energy supersymmetric models, LHC…

高能物理 - 唯象学 · 物理学 2008-11-26 Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

A kinetic mixing between the axion and the inflaton allows for a production of axion dark matter even if the inflationary Hubble scale is smaller than the zero-temperature axion mass. We analyze the axion dynamics in this recently…

高能物理 - 唯象学 · 物理学 2020-09-10 Takeshi Kobayashi , Lorenzo Ubaldi

The dark dimension scenario, which is motivated from Swampland principles and predicts a single micron scale extra dimension, suggests a consistent framework for the dark sector of the universe. We consider the implications of this scenario…

高能物理 - 理论 · 物理学 2024-07-18 Naomi Gendler , Cumrun Vafa

It was shown in ref. [1] that cold dark matter axions reach thermal contact with baryons, and therefore cool them, shortly after the axions thermalize among themselves and form a Bose-Einstein condensate. The recent observation by the EDGES…

宇宙学与河外天体物理 · 物理学 2018-08-02 Pierre Sikivie

By coupling to both the Higgs and electroweak gauge sectors, an axion can generate the matter-antimatter asymmetry in the universe via electroweak baryogenesis when the axion decay constant lies within the range of approximately $10^5$ and…

高能物理 - 唯象学 · 物理学 2025-02-11 Kwang Sik Jeong , Ju Hyeong Kang , Shota Nakagawa

We discuss two cosmological issues in a generic gauge-mediated supersymmetry (SUSY)-breaking model, namely the Universe's baryon asymmetry and the gravitino dark-matter density. We show that both problems can be simultaneously solved if…

高能物理 - 唯象学 · 物理学 2009-11-07 Masaaki Fujii , T. Yanagida

Mixed dark matter scenario can reconcile the COBE data and the observed large scale structure. So far the massive neutrino with a mass of a few eV has been the only discussed candidate for the hot dark matter component. We point out that…

高能物理 - 唯象学 · 物理学 2008-11-26 Takeo Moroi , Hitoshi Murayama

An analysis is given of interacting dark energy and dark matter where the dark energy is assumed to be an ultralight axionic field with a pseudo-Nambu-Goldstone Boson potential which is in general a superposition of $N$ number of cosine…

宇宙学与河外天体物理 · 物理学 2025-12-01 Amin Aboubrahim , Andrew H. Giman , Pran Nath

The search for supersymmetric partners at Large Hadron Collider revealed negative result. Though, strictly speaking, it does not exclude low energy supersymmetry, but still it leads to strong constraints of the parameter space. Therefore…

高能物理 - 唯象学 · 物理学 2024-01-26 E. V. Arbuzova

An axion rotating in field space can produce dark photons in the early universe via tachyonic instability. This explosive particle production creates a background of stochastic gravitational waves that may be visible at pulsar timing arrays…

高能物理 - 唯象学 · 物理学 2022-01-05 Raymond T. Co , Keisuke Harigaya , Aaron Pierce

We examine the hypothesis of decaying heavy dark matter (HDM) in the context of the IceCube highest energy neutrino events and recent limits on the diffuse flux of high-energy photons. We consider dark matter (DM) particles $X$ of mass…

高能天体物理现象 · 物理学 2018-12-04 M. Kachelriess , O. E. Kalashev , M. Yu. Kuznetsov

We examine non-thermal dark matter production from a late-decaying scalar field, with a particular attention on non-renormalizable operators of D=5 through which the scalar field decays into the standard model particles and their…

高能物理 - 唯象学 · 物理学 2009-11-11 Motoi Endo , Fuminobu Takahashi

Light axions ($m_a \lesssim 10^{-10}$ eV) can form dense clouds around rapidly rotating astrophysical black holes via a mechanism known as rotational superradiance. The coupling between axions and photons induces a parametric resonance,…

宇宙学与河外天体物理 · 物理学 2020-11-25 Diego Blas , Samuel J. Witte

The cold dark matter (CDM) paradigm provides a remarkably good description of the Universe's large-scale structure. However, some discrepancies exist between its predictions and observations at very small sub-galactic scales. To address…

宇宙学与河外天体物理 · 物理学 2024-01-04 Atrideb Chatterjee , Sourav Mitra , Amrita Banerjee

We discuss several aspects of astroparticle physics pertaining to a new model with MeV cold dark matter particles, which annihilate to electron-positron pairs in a manner yielding the correct CDM density required today, and explaining the…

高能物理 - 唯象学 · 物理学 2010-10-27 Chen Jacoby , Shmuel Nussinov