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A number of observed phenomena in high energy physics and cosmology lack their resolution within the Standard Model of particle physics. These puzzles include neutrino oscillations, baryon asymmetry of the universe and existence of dark…

高能物理 - 唯象学 · 物理学 2008-12-18 Mikhail Shaposhnikov

Short baseline neutrino oscillation experiments have shown hints of the existence of additional sterile neutrinos in the eV mass range. Such sterile neutrinos are incompatible with cosmology because they suppress structure formation unless…

宇宙学与河外天体物理 · 物理学 2015-03-30 Maria Archidiacono , Steen Hannestad , Rasmus Sloth Hansen , Thomas Tram

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

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether…

高能物理 - 唯象学 · 物理学 2018-05-09 Andres Olivares-Del Campo , Celine Boehm , Sergio Palomares-Ruiz , Silvia Pascoli

We identify the range of parameters for which the sterile neutrinos can simultaneously explain the cosmological dark matter and the observed velocities of pulsars. To satisfy all cosmological bounds, the relic sterile neutrinos must be…

高能物理 - 唯象学 · 物理学 2007-05-23 Alexander Kusenko

Taken at face value, current experimental data indicate the existence of a new particle, the sterile neutrino, which must be a singlet under the Standard Model gauge group. Although they are not detectable through traditional means, such…

高能物理 - 唯象学 · 物理学 2007-05-23 Mitesh Patel , George M. Fuller

While the standard model accurately describes data at the electroweak scale without inclusion of gravity, beyond the standard model physics is increasingly intertwined with gravitational phenomena and cosmology. Thus gravity mediated…

高能物理 - 唯象学 · 物理学 2024-02-07 Pran Nath

We add a singlet right handed neutrino plus a charged and a neutral singlet scalars to the standard model. This extension includes a discrete symmetry such that we obtain a heavy sterile neutrino which couples only to the electron and the…

高能物理 - 唯象学 · 物理学 2010-12-09 F. S. Queiroz , C. A. de S. Pires , P. S. Rodrigues da Silva

The presence of light sterile neutrinos is one of the unanswered questions of particle physics. The cosmological counterpart is represented by dark radiation, i.e.\ any form of radiation present in the early Universe besides photons and…

高能物理 - 唯象学 · 物理学 2022-03-16 Maria Archidiacono , Stefano Gariazzo

We consider an extended seesaw model which generates active neutrino masses via the usual type-I seesaw and leads to a large number of massless fermions as well as a sterile neutrino dark matter (DM) candidate in the $\mathcal{O}(10-100)…

高能物理 - 唯象学 · 物理学 2025-04-22 Cristina Benso , Thomas Schwetz , Drona Vatsyayan

An extension of the Standard Model by extra scalar singlets was considered. Theoretical (unitarity, vacuum stability, triviality) and cosmological (dark matter relic abundance, direct detection experiments, constraints on dark matter…

高能物理 - 唯象学 · 物理学 2013-10-14 Aleksandra Drozd , Bohdan Grzadkowski , Jose Wudka

The cosmological significance of the neutralino sector is studied for a class of models in which electroweak symmetry breaking is seeded by a gauge singlet. Extensive use is made of the renormalisation group equations to significantly…

高能物理 - 唯象学 · 物理学 2011-02-16 S. A. Abel , S. Sarkar , I. B. Whittingham

Sterile neutrinos only interact with the Standard Model through the neutrino sector, and thus represent a simple dark matter (DM) candidate with many potential astrophysical and cosmological signatures. Recently, sterile neutrinos produced…

宇宙学与河外天体物理 · 物理学 2023-11-16 Rui An , Vera Gluscevic , Ethan O. Nadler , Yue Zhang

In usual particle models, sterile neutrinos can account for the dark matter of the Universe only if they have masses in the keV range and are warm dark matter. Stringent cosmological and astrophysical bounds, in particular imposed by X-ray…

高能物理 - 唯象学 · 物理学 2010-04-14 Graciela B. Gelmini , Efunwande Osoba , Sergio Palomares-Ruiz

We explore the range of parameters for dark-matter sterile neutrinos in an extention of the Minimal Standard Model by three singlet fermions with masses below the electroweak scale (the $\nu$MSM). This simple model can explain a wide range…

高能物理 - 唯象学 · 物理学 2008-11-26 Takehiko Asaka , Mikhail Shaposhnikov , Alexander Kusenko

One of the simplest extensions of the Standard Model that explains the observed abundance of dark matter is the inert doublet model. In this theory a discrete symmetry ensures that the neutral component of an additional electroweak doublet…

高能物理 - 唯象学 · 物理学 2010-04-21 Prateek Agrawal , Ethan M. Dolle , Christopher A. Krenke

We investigate observable cosmological aspects of sterile neutrino dark matter produced via the freeze-in mechanism. The study is performed in a framework that admits many cosmologically interesting variations: high temperature production…

高能物理 - 唯象学 · 物理学 2017-06-15 Samuel B. Roland , Bibhushan Shakya

We suggest that recent neutrino puzzles that are the solar and atmospheric neutrino deficits as well as the possible neutrino oscillations reported by the LSND experiment and the possibility of massive neutrinos providing the hot component…

高能物理 - 唯象学 · 物理学 2009-10-28 Z. Berezhiani , R. N. Mohapatra

In this paper, a cosmological model is considered, in which dark matter is emitted by T-symmetric quasi-black holes distributed over galaxies. Low energy photons and neutrinos are taken as candidates for dark matter particles. Photon case…

综合物理 · 物理学 2024-01-08 Igor Nikitin

We show that a self-consistent and coupled treatment of the weak decoupling, big bang nucleosynthesis, and photon decoupling epochs can be used to provide new insights and constraints on neutrino sector physics from high-precision…

宇宙学与河外天体物理 · 物理学 2015-05-27 E. Grohs , G. M. Fuller , C. T. Kishimoto , M. W. Paris
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