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We reappraise the viability of asymmetric dark matter (ADM) realized as a Dirac fermion coupling dominantly to the Standard Model fermions. Treating the interactions of such a DM particle with quarks/leptons in an effective-interactions…

高能物理 - 唯象学 · 物理学 2024-07-19 Arnab Roy , Basudeb Dasgupta , Monoranjan Guchait

We compute the bounds on the dark matter (DM) annihilation cross section using the most recent Cosmic Microwave Background measurements from WMAP9, SPT'11 and ACT'10. We consider DM with mass in the MeV-TeV range annihilating 100% into…

宇宙学与河外天体物理 · 物理学 2013-09-13 Laura Lopez-Honorez , Olga Mena , Sergio Palomares-Ruiz , Aaron C. Vincent

An effective interaction approach is used to describe the interactions between the spin 0 or spin 1/2 dark matter particle and the degrees of freedom of the standard model. This approach is applicable to those models in which the dark…

高能物理 - 唯象学 · 物理学 2015-06-03 Kingman Cheung , Po-Yan Tseng , Yue-Lin S. Tsai , Tzu-Chiang Yuan

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 analyze cosmic microwave background (CMB) data to constrain the mass and interaction strengths of thermally-produced dark matter (DM) in a self-consistent manner, simultaneously taking into account the cosmological effects of its mass…

宇宙学与河外天体物理 · 物理学 2024-06-14 Rui An , Kimberly K. Boddy , Vera Gluscevic

We explore the phenomenology of Elastically Decoupling Relic (ELDER) dark matter. ELDER is a thermal relic whose present density is determined primarily by the cross-section of its elastic scattering off Standard Model (SM) particles.…

高能物理 - 唯象学 · 物理学 2018-06-14 Eric Kuflik , Maxim Perelstein , Nicolas Rey-Le Lorier , Yu-Dai Tsai

The null signal from collider and dark matter (DM) direct detector experiments makes the interaction between DM and visible matter too small to reproduce the correct relic density for many thermal DM models. The remaining parameter space…

高能物理 - 唯象学 · 物理学 2022-05-04 Jie-Cheng Feng , Xian-Wei Kang , Chih-Ting Lu , Yue-Lin Sming Tsai , Feng-Shou Zhang

A comprehensive analysis of cosmological and collider constraints is presented for three simplified models characterised by a dark matter candidate (real scalar, Majorana fermion and real vector) and a coloured mediator (fermion, scalar and…

高能物理 - 唯象学 · 物理学 2021-04-22 Chiara Arina , Benjamin Fuks , Luca Mantani , Hanna Mies , Luca Panizzi , Jakub Salko

We propose a Two-Loop induced radiative neutrino model with hidden gauged $U(1)$ symmetry, in which a dark matter of Dirac fermion arises. The relic density gets contribution from annihilation and semi-annihilation due to a residual…

高能物理 - 唯象学 · 物理学 2020-02-12 Haiying Cai

The status of the constrained minimal supersymmetric standard model (CMSSM) will be discussed in light of our current understanding of the relic density after WMAP. A global likelihood analysis of the model is performed including data from…

高能物理 - 唯象学 · 物理学 2007-05-23 Keith A. Olive

The identity of Dark Matter (DM) is one of the most captivating topics in particle physics today. The R-parity conserving Minimal Supersymmetric Standard Model (MSSM), which naturally provides a DM candidate in the form of the lightest…

高能物理 - 唯象学 · 物理学 2018-01-15 Carlos Ávila , Andrés Flórez , Alfredo Gurrola , Dale Julson , Savanna Starko

Chemical equilibrium is a commonly made assumption in the freeze-out calculation of coannihilating dark matter. We explore the possible failure of this assumption and find a new conversion-driven freeze-out mechanism. Considering a…

高能物理 - 唯象学 · 物理学 2017-11-20 Mathias Garny , Jan Heisig , Benedikt Lülf , Stefan Vogl

We introduce a model of dark matter (DM) where the DM is a composite of a spontaneously broken conformal field theory. The DM is a thermal relic with its abundance determined by the freeze-out of annihilations to dilatons, the Goldstone…

高能物理 - 唯象学 · 物理学 2023-09-13 Steven Ferrante , Ameen Ismail , Seung J. Lee , Yunha Lee

We investigate the phenomenology of a simplified model with a Majorana fermion as dark matter candidate which interacts with Standard Model quarks via a colour-charged coannihilation partner. Recently it has been realized that…

高能物理 - 唯象学 · 物理学 2019-03-19 S. Biondini , S. Vogl

We explore dark matter in the Finely Tuned Minimal Supersymmetric Standard model recently proposed by Arkani-Hamed and Dimopoulos. Relative to the MSSM, there are fewer particles at freeze-out, so the calculation of the relic abundance…

高能物理 - 唯象学 · 物理学 2008-11-26 Aaron Pierce

Dark Matter particles with inelastic interactions are ubiquitous in extensions of the Standard Model, yet remain challenging to fully probe with existing strategies. We propose a series of powerful searches at hadron and lepton colliders…

高能物理 - 唯象学 · 物理学 2016-03-30 Eder Izaguirre , Gordan Krnjaic , Brian Shuve

We present a dark sector model based on gauging the $L_\mu - L_\tau$ symmetry that addresses anomalies in $b \rightarrow s \mu^+ \mu^-$ decays and that features a particle dark matter candidate. The dark matter particle candidate is a…

高能物理 - 唯象学 · 物理学 2017-03-14 Wolfgang Altmannshofer , Stefania Gori , Stefano Profumo , Farinaldo S. Queiroz

New particles in theories beyond the standard model can manifest as stable relics that interact strongly with visible matter and make up a small fraction of the total dark matter abundance. Such particles represent an interesting physics…

高能物理 - 唯象学 · 物理学 2023-07-10 David McKeen , David E. Morrissey , Maxim Pospelov , Harikrishnan Ramani , Anupam Ray

We derive joint constraints on the warm dark matter (WDM) half-mode scale by combining the analyses of a selection of astrophysical probes: strong gravitational lensing with extended sources, the Lyman-$\alpha$ forest, and the number of…