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The standard cold dark matter cosmological model, while successful in explaining the observed large scale structure of the Universe, tends to overpredict structure on small scales. It has been proposed this problem may be alleviated in a…

高能物理 - 唯象学 · 物理学 2011-03-21 Nicole F. Bell , Ahmad J. Galea , Raymond R. Volkas

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold…

宇宙学与河外天体物理 · 物理学 2020-08-04 Ivan de Martino , Sankha S. Chakrabarty , Valentina Cesare , Arianna Gallo , Luisa Ostorero , Antonaldo Diaferio

Supersymmetry offers a cold dark matter candidate, provided that lepton number is {\em not violated by an odd number of units}. On the other hand, lepton number violation by even (two) units gives us an attractive mechanism of neutrino mass…

高能物理 - 唯象学 · 物理学 2008-11-26 Biswarup Mukhopadhyaya , Soumitra SenGupta , Raghavendra Srikanth

We study a seesaw-type extension of the Standard Model in which the symmetry group is enlarged by a global U(1). We introduce adequate scalar and fermion representations which naturally explain the smallness of neutrino masses. With the…

高能物理 - 唯象学 · 物理学 2011-12-19 François-Xavier Josse-Michaux , Emiliano Molinaro

A possible extension of the Standard Model to include lepton number as local gauge symmetry is investigated. In such a model, anomalies are canceled by two extra fermions doublet. After leptonic gauge symmetry spontaneously broken, three…

高能物理 - 唯象学 · 物理学 2011-01-03 Wei Chao

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

The standard model of particle physics is marvelously successful. However, it is obviously not a complete or final theory. I shall argue here that the structure of the standard model gives some quite concrete, compelling hints regarding…

高能物理 - 唯象学 · 物理学 2009-10-28 Frank Wilczek

We propose a minimal model based on lepton number symmetry (and violation), to address a common origin of baryon asymmetry, dark matter and neutrino mass generation. The model consists of a vector like fermion to constitute the dark sector,…

高能物理 - 唯象学 · 物理学 2022-10-12 Subhaditya Bhattacharya , Rishav Roshan , Arunansu Sil , Drona Vatsyayan

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

Supersymmetric scenarios incorporating thermal leptogenesis as the origin of the observed matter-antimatter asymmetry generically predict abundances of the primordial elements which are in conflict with observations. In this paper we…

高能物理 - 唯象学 · 物理学 2011-07-28 Andrea De Simone , Mathias Garny , Alejandro Ibarra , Christoph Weniger

We investigate the dark matter and the cosmological baryon asymmetry in a simple theory where baryon (B) and lepton (L) number are local gauge symmetries that are spontaneously broken. In this model, the cold dark matter candidate is the…

高能物理 - 唯象学 · 物理学 2015-03-17 Timothy R. Dulaney , Pavel Fileviez Perez , Mark B. Wise

Our standard model of the Universe predicts the distribution of dark matter to $1\%$ at the scales needed for upcoming experiments, yet our predictions for how the luminous matter -- which has interactions besides gravity -- is distributed…

高能物理 - 理论 · 物理学 2025-03-03 Nora Elisa Chisari

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

星系天体物理 · 物理学 2020-03-10 Paolo Salucci , Nicola Turini

In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

高能物理 - 唯象学 · 物理学 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

We study the possibility to describe dark matter in a model of the universe with two scale factors and a non-standard Poisson bracket structure characterized by the deformation parameter \kappa. The dark matter evolution is analyzed in the…

高能物理 - 唯象学 · 物理学 2023-08-16 Carlos Maldonado , Fernando Mendez

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

高能物理 - 唯象学 · 物理学 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

In this Letter, we propose a new possible connection between dark matter relic density and baryon asymmetry of the universe. The portal between standard model sector and dark matter not only controls the relic density and detections of dark…

高能物理 - 唯象学 · 物理学 2015-05-30 Talal Ahmed Chowdhury , Miha Nemevsek , Goran Senjanovic , Yue Zhang

We present kinematically forbidden dark matter annihilations into Standard Model leptons. This mechanism precisely selects the dark matter mass that gives the observed relic abundance. This is qualitatively different from existing models of…

高能物理 - 唯象学 · 物理学 2021-06-21 Raffaele Tito D'Agnolo , Di Liu , Joshua T. Ruderman , Po-Jen Wang

Last year observations had a profound impact on our views on the amount and nature of dark matter in the universe. We give a brief review of the recent history of dark matter models beyond the pure cold dark matter universe. In view of the…

高能物理 - 唯象学 · 物理学 2007-05-23 Antonio Masiero , Francesca Rosati

Dark matter is postulated as a light fermion in two natural scenarios as the outcome of a softly broken discrete symmetry. It is produced from the naturally suppressed decay of the standard-model Higgs boson through the freeze-in mechanism.

高能物理 - 唯象学 · 物理学 2024-09-25 Ernest Ma