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A very simple production mechanism of feebly interacting dark matter (DM) that rarely annihilates is thermal production, which predicts the DM mass around eV. This has been widely known as the hot DM scenario. Despite there are several…

高能物理 - 唯象学 · 物理学 2023-06-07 Wen Yin

We propose to search for axion dark matter via the oscillating electric dipole moments that axions induce in atoms and molecules. These moments are produced through the intrinsic oscillating electric dipole moments of nucleons and through…

原子物理 · 物理学 2015-11-16 Benjamin M. Roberts , Yevgeny V. Stadnik , Victor V. Flambaum , Vladimir A. Dzuba

Dark matter could be a thermal relic comprised of strongly interacting massive particles (SIMPs), where $3 \rightarrow 2$ interactions set the relic abundance. Such interactions generically arise in theories of chiral symmetry breaking via…

高能物理 - 唯象学 · 物理学 2019-01-08 Yonit Hochberg , Eric Kuflik , Robert McGehee , Hitoshi Murayama , Katelin Schutz

Generating small sterile neutrino masses via the same seesaw mechanism that suppresses active neutrino masses requires a specific structure in the neutral fermion mass matrix. We present a model where this structure is enforced by a new…

高能物理 - 唯象学 · 物理学 2013-06-03 Julian Heeck , He Zhang

We investigate cosmological implications of an energy density contribution arising by elastic dark matter self-interactions. Its scaling behaviour shows that it can be the dominant energy contribution in the early universe. Constraints from…

宇宙学与河外天体物理 · 物理学 2011-04-06 Rainer Stiele , Tillmann Boeckel , Jurgen Schaffner-Bielich

If the dark matter is produced in the early universe prior to Big Bang nucleosynthesis, a modified cosmological history can drastically affect the abundance of relic dark matter particles. Here, we assume that an additional species to…

高能物理 - 唯象学 · 物理学 2018-02-26 Francesco D'Eramo , Nicolas Fernandez , Stefano Profumo

A new scenario for creation of galactic magnetic fields is proposed which is operative at the cosmological epoch of the galaxy formation, and which relies on unconventional properties of dark matter. Namely, it requires existence of feeble…

宇宙学与河外天体物理 · 物理学 2013-12-09 Zurab Berezhiani , A. D. Dolgov , I. I. Tkachev

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…

高能物理 - 实验 · 物理学 2025-06-24 Vindhyawasini Prasad

In this paper we present a novel mechanism for producing the observed Dark Matter(DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities…

高能物理 - 唯象学 · 物理学 2021-01-15 Aleksandr Azatov , Miguel Vanvlasselaer , Wen Yin

Recently, Madsen has argued that relativistic decays of massive neutrinos into lighter fermions and bosons may lead, via thermalization, to the formation of a Bose condensate. If correct, this could generate mixed hot and cold dark matter,…

高能物理 - 唯象学 · 物理学 2009-10-22 N. Kaiser , R. A. Malaney , G. D. Starkman

We introduce a novel mechanism where the kinetic energy of a rotating axion can be dissipated by the interactions with dark magnetic monopoles. This mechanism leads to a framework where the QCD axion and dark monopoles account for the dark…

高能物理 - 唯象学 · 物理学 2025-11-14 Raymond T. Co , Keisuke Harigaya , Isaac R. Wang , Huangyu Xiao

The vector portal/kinetic mixing simplified model of dark matter, in which thermal dark matter of a mass ranging from a few MeV to a few GeV can be realized with a dark-sector $U(1)$, relies on a small kinetic mixing term between this dark…

高能物理 - 唯象学 · 物理学 2023-08-16 George N. Wojcik

We study a scenario in which the dilaton, a pseudo-Goldstone boson of the spontaneous breaking of conformal symmetry, provides a portal between dark matter and the visible sector. We consider the low-energy description of the theory in…

高能物理 - 唯象学 · 物理学 2015-06-23 Aielet Efrati , Eric Kuflik , Shmuel Nussinov , Yotam Soreq , Tomer Volansky

We construct a self-interacting dark matter model that could simultaneously explain the observed muon anomalous magnetic moment. It is based on a gauged U$(1)_{L_{\mu} - L_{\tau}}$ extension of the standard model, where we introduce a…

高能物理 - 唯象学 · 物理学 2018-07-31 Ayuki Kamada , Kunio Kaneta , Keisuke Yanagi , Hai-Bo Yu

A new understanding of the stability of self-interacting dark matter is pointed out, based on the simplest spontaneously broken Abelian $U(1)$ gauge model with one complex scalar and one Dirac fermion. The key is the imposition of dark…

高能物理 - 唯象学 · 物理学 2017-08-23 Ernest Ma

In this work we complete a model independent analysis of dark matter constraining its mass and interaction strengths with data from astro- and particle physics experiments. We use the effective field theory framework to describe…

高能物理 - 唯象学 · 物理学 2015-06-19 Csaba Balázs , Tong Li , Jayden L. Newstead

While the evidence for dark matter continues to grow, the nature of the dark matter remains a mystery. A dark $U(1)_D$ gauge theory can have a small kinetic mixing with the visible photon which provides a portal to the dark sector. Magnetic…

高能物理 - 唯象学 · 物理学 2020-01-01 John Terning , Christopher B. Verhaaren

We consider the thermal effects into the evaluation of the dark matter production process. With the assistance of the right handed neutrinos, the freeze-in massive particle dark matter production history can be modified by the two-step…

高能物理 - 唯象学 · 物理学 2018-12-26 Ligong Bian , Yi-Lei Tang

A possible connection between the cosmological baryon asymmetry, dark matter and vector-like fermions is investigated. In this scenario an asymmetry generated through baryogenesis or leptogenesis (in the vector-like matter sector) connects…

高能物理 - 唯象学 · 物理学 2013-05-22 Pavel Fileviez Perez , Mark B. Wise

Big-Bang nucleosynthesis (BBN) represents one of the earliest phenomena that can lead to observational constraints on the early Universe properties. It is well-known that many important mechanisms and phase transitions occurred before BBN.…

高能物理 - 唯象学 · 物理学 2018-12-03 A. Arbey , J. Ellis , F. Mahmoudi , G. Robbins