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We point out a selection rule for enhancement (suppression) of odd (even) partial waves of dark matter coannihilation or annihilation using Sommerfeld effect. Using this, the usually velocity-suppressed p-wave annihilation can dominate the…

高能物理 - 唯象学 · 物理学 2017-06-30 Anirban Das , Basudeb Dasgupta

The relic density of TeV-scale wino-like neutralino dark matter in the MSSM is subject to potentially large corrections as a result of the Sommerfeld effect. A recently developed framework enables us to calculate the Sommerfeld-enhanced…

高能物理 - 唯象学 · 物理学 2016-04-20 M. Beneke , A. Bharucha , F. Dighera , C. Hellmann , A. Hryczuk , S. Recksiegel , P. Ruiz-Femenia

We study the impact of the Sommerfeld enhancement on the thermal relic density of the lightest neutralino in the case of large co-annihilation effects with a scalar particle. The proper way of including the Sommerfeld effect in this case is…

高能物理 - 唯象学 · 物理学 2015-05-27 Andrzej Hryczuk

We explore the viability of a boson dark matter candidate with an asymmetry between the number densities of particles and antiparticles. A simple thermal field theory analysis confirms that, under certain general conditions, this component…

宇宙学与河外天体物理 · 物理学 2016-04-27 Anthony Aguirre , Alberto Diez-Tejedor

A solution to the Boltzmann equation governing the thermal relic abundance of cold dark matter is constructed by matched asymptotic approximations. The approximation of the relic density is an asymptotic series valid when the abundance does…

高能物理 - 唯象学 · 物理学 2021-07-16 Logan A. Morrison , Hiren H. Patel , Jaryd F. Ulbricht

Based on the cosmological observations, the baryon and dark matter energy densities are similar. There may exist an asymmetry between the dark matter particles and their corresponding anti--particles. We review the relic density of…

高能物理 - 唯象学 · 物理学 2023-10-06 Qiu Sujuan , Hoernisa Iminniyaz

Approximate analytical solutions of the Boltzmann equation for particles that are either extremely relativistic or non-relativistic when they decouple from the thermal bath are well established. However, no analytical formula for the relic…

高能物理 - 唯象学 · 物理学 2009-09-02 Manuel Drees , Mitsuru Kakizaki , Suchita Kulkarni

In existing dark matter models with global symmetries the relic abundance of dark matter is either equal to that of anti-dark matter (thermal WIMP), or vastly larger, with essentially no remaining anti-dark matter (asymmetric dark matter).…

高能物理 - 唯象学 · 物理学 2015-05-27 Michael L. Graesser , Ian M. Shoemaker , Luca Vecchi

We investigate the implication of unparticle exchange for the possible Sommerfeld enhancement in dark matter annihilation process. Assuming the unparticle exchange during WIMP collision, we solve the Schr\rm\ddot{o}dinger equation for the…

高能物理 - 唯象学 · 物理学 2010-04-14 Chuan-Hung Chen , C. S. Kim

The relic density of a cold dark matter (CDM) candidate is calculated in the context of three non-standard cosmological scenaria and its value is compared with the one obtained in the standard regime. In particular, we consider the…

高能物理 - 唯象学 · 物理学 2016-11-09 C. Pallis

The $\Lambda$CDM model, while successful on large cosmological scales, faces challenges on small scales. A promising solution posits that dark matter (DM) exhibits strong self-interaction, enhanced through the narrow resonance or Sommerfeld…

高能物理 - 唯象学 · 物理学 2026-05-21 Shao-Song Tang , Murat Abdughani

We investigate the relic abundance of dark matter from coannihilation in non-standard cosmological scenarios. We explore the effect of coannihilation on the relic density of dark matter and freeze out temperature in quintessence model with…

高能物理 - 唯象学 · 物理学 2024-02-13 Fangyu Liu , Hoernisa Iminniyaz

We study the effect of the elastic scattering on the non-thermal WIMP, which is produced by direct decay of heavy particles at the end of reheating. The non-thermal WIMP becomes important when the reheating temperature is well below the…

高能物理 - 唯象学 · 物理学 2017-03-15 Hyungjin Kim , Jeong-Pyong Hong , Chang Sub Shin

Dark matter with Sommerfeld-enhanced annihilation has been proposed to explain observed cosmic ray positron excesses in the 10 GeV to TeV energy range. We show that the required enhancement implies thermal relic densities that are too small…

高能物理 - 唯象学 · 物理学 2010-04-29 Jonathan L. Feng , Manoj Kaplinghat , Hai-Bo Yu

The relic abundance of the dark matter (DM) particle $d$ is studied in a secluded DM scenario, in which the $d$ number decreasing process dominantly occurs not through the pair annihilation of $d$ into the standard model particles, but via…

高能物理 - 唯象学 · 物理学 2017-03-08 Shohei Okawa , Masaharu Tanabashi , Masato Yamanaka

We investigate the effect of a braneworld expansion era on the relic density of asymmetric dark matter. We find that the enhanced expansion rate in the early universe predicted by the Randall-Sundrum II (RSII) model leads to earlier…

宇宙学与河外天体物理 · 物理学 2015-06-19 Michael T. Meehan , Ian B. Whittingham

We present a model with dark matter in an anomaly-mediated supersymmetry breaking hidden sector with a U(1)xU(1) gauge symmetry. The symmetries of the model stabilize the dark matter and forbid the introduction of new mass parameters. As a…

高能物理 - 唯象学 · 物理学 2013-05-30 Jonathan L. Feng , Vikram Rentala , Ze'ev Surujon

We revisit the calculation of relic density of dark matter particles co-annihilating with a top or bottom partner, by properly including the QCD bound-states (onia) effects of the colored partners, as well as the relevant electroweak…

高能物理 - 唯象学 · 物理学 2017-07-19 Wai-Yee Keung , Ian Low , Yue Zhang

We present an analysis of the Sommerfeld enhancement to dark matter annihilation in the presence of an excited state, where the interaction inducing the enhancement is purely off-diagonal, such as in models of exciting or inelastic dark…

高能物理 - 唯象学 · 物理学 2010-03-09 Tracy R. Slatyer

In Scalar-Tensor theories of gravity, the expansion rate of the universe in the past may differ considerably from the standard one. After imposing the constraints coming from nucleosynthesis, CMB, type Ia supernovae, and solar system tests…

天体物理学 · 物理学 2007-05-23 R. Catena , N. Fornengo , A. Masiero , M. Pietroni , F. Rosati