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相关论文: Asymmetric accidental composite dark matter

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We study the possibility of cogenesis of baryon and dark matter (DM) from the out-of-equilibrium CP violating decay of right handed neutrino (RHN) that are dominantly of non-thermal origin. While the RHN and its heavier partners can take…

高能物理 - 唯象学 · 物理学 2022-03-30 Basabendu Barman , Debasish Borah , Suruj Jyoti Das , Rishav Roshan

We consider a chiral gauge theory from which light composite Dirac neutrinos dynamically emerge, augmented by a QCD axion to solve the strong CP problem. We show that an interplay between the composite sector and the axion can also…

高能物理 - 唯象学 · 物理学 2022-02-02 Sabyasachi Chakraborty , Tae Hyun Jung , Takemichi Okui

A dark QCD sector is a relatively minimal extension of the Standard Model (SM) that admits Dark Matter (DM) candidates but requires no portal to the visible sector beyond gravitational interactions: A "nightmare scenario" for DM detection.…

高能物理 - 唯象学 · 物理学 2021-06-02 Logan Morrison , Stefano Profumo , Dean J. Robinson

Sterile neutrinos as source of mass and flavor mixing of active neutrinos as well as genesis of dark matter (DM) and matter-antimatter asymmetry have gained special interest. Here we study the case of the Standard Model (SM) extended with…

高能物理 - 唯象学 · 物理学 2024-11-27 Ernesto A. Matute

We review a testable dark matter (DM) model outside of the standard WIMP paradigm. The model is unique in a sense that the observed ratio $\Omega_{\rm dark} \simeq \Omega_{\rm visible}$ for visible and dark matter densities finds its…

高能物理 - 唯象学 · 物理学 2017-04-05 Ariel Zhitnitsky

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number $B_X$, and $\sigma^{\rm annih}_{\bar{X}} < \sigma^{\rm…

高能物理 - 唯象学 · 物理学 2007-05-23 Glennys R. Farrar , Gabrijela Zaharijas

We study the effect of a first-order phase transition in a confining $SU(N)$ dark sector with heavy dark quarks. The baryons of this sector are the dark matter candidate. During the confinement phase transition the heavy quarks are trapped…

高能物理 - 唯象学 · 物理学 2021-11-24 Pouya Asadi , Eric David Kramer , Eric Kuflik , Gregory W. Ridgway , Tracy R. Slatyer , Juri Smirnov

We propose a new mechanism to simultaneously explain the observed dark matter abundance and the baryon asymmetry of the Universe. The mechanism is based on the Filtered Dark Matter scenario, where dark matter particles acquire a large mass…

高能物理 - 唯象学 · 物理学 2022-08-24 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht , Yotam Soreq

Increasingly stringent limits from LHC searches for new physics, coupled with lack of convincing signals of weakly interacting massive particle (WIMP) in dark matter searches, have tightly constrained many realizations of the standard…

高能物理 - 唯象学 · 物理学 2015-01-27 Howard Baer , Ki-Young Choi , Jihn E. Kim , Leszek Roszkowski

I suggest an effective model between the GUT and the electroweak scale. It only introduces the two symmetries of $U(1)_{B-L}$ and $U(1)_{D}$ besides the SM groups. The two symmetries are individually broken at the reheating temperature of…

高能物理 - 唯象学 · 物理学 2016-09-21 Wei-Min Yang

We illustrate, via a simplified model, a scenario in which the baryon-asymmetry and, possibly the dark matter component of the Universe are simultaneously generated by the decay of a WIMP-like mother particle, in turn produced non-thermally…

高能物理 - 唯象学 · 物理学 2026-04-15 Giorgio Arcadi , Sarif Khan , Agnese Mariotti

We study a dark matter (DM) model offering a very natural explanation of two (naively unrelated) problems in cosmology: the observed relation $\Omega_{\rm DM}\sim\Omega_{\rm visible}$ and the observed asymmetry between matter and antimatter…

高能物理 - 唯象学 · 物理学 2018-02-21 Shuailiang Ge , Xunyu Liang , Ariel Zhitnitsky

We examine cosmological, astrophysical and collider constraints on thermal dark matter (DM) with mass mX in the range 1 MeV to 10 GeV. Cosmic microwave background (CMB) observations, which severely constrain light symmetric DM, can be…

高能物理 - 唯象学 · 物理学 2012-12-12 Tongyan Lin , Hai-Bo Yu , Kathryn M. Zurek

Indirect searches of Dark Matter (DM), in conjugation with `missing track searches' at the collider seem to confine SU(2)$_L$ fermion triplet DM (FTDM) mass within a narrow range around 1 TeV. The canonical picture of the pure FTDM is in…

高能物理 - 唯象学 · 物理学 2023-08-21 Anirban Biswas , Mainak Chakraborty , Sarif Khan

The extension of the Standard model (SM) with three heavy right handed neutrinos, a complex scalar and the gauged $U(1)_{\rm B-L}$ symmetry (the minimal $B-L$ model) is considered the most compelling minimal one: the presence and the…

高能物理 - 唯象学 · 物理学 2021-01-19 Gongjun Choi , Tsutomu T. Yanagida , Norimi Yokozaki

We present a supersymmetric extension of the Standard Model (USSM-A) with an anomalous U(1) and Stueckelberg axions for anomaly cancellation, generalizing similar non-supersymmetric constructions. The model, built by a bottom-up approach,…

高能物理 - 唯象学 · 物理学 2009-08-13 Claudio Coriano' , Marco Guzzi , Antonio Mariano , Simone Morelli

We introduce a novel dark matter scenario where the visible sector and the dark sector share a common asymmetry. The two sectors are connected through an unstable mediator with baryon number one, allowing the standard model baryon asymmetry…

高能物理 - 唯象学 · 物理学 2016-03-16 Nayara Fonseca , Lina Necib , Jesse Thaler

We propose an extension of the standard model (SM) by including a dark sector comprising of three generations of heavy right-handed neutrinos, a singlet scalar and a singlet Dirac fermion, where the latter two particles are stable and are…

高能物理 - 唯象学 · 物理学 2020-01-07 Nimmala Narendra , Sudhanwa Patra , Narendra Sahu , Sujay Shil

We study generation of baryon number asymmetry and both abundance of dark matter and dark energy on the basis of global symmetry and its associating flat directions in a supersymmetric model. We assume the existence of a model independent…

天体物理学 · 物理学 2009-11-13 Daijiro Suematsu

We study a testable dark matter (DM) model outside of the standard WIMP paradigm in which the observed ratio $\Omega_{\rm dark} \simeq \Omega_{\rm visible}$ for visible and dark matter densities finds its natural explanation as a result of…

高能物理 - 唯象学 · 物理学 2016-10-12 Xunyu Liang , Ariel Zhitnitsky