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The simplest model that can accomodate a viable nonbaryonic dark matter candidate is the standard electroweak theory with the addition of right-handed or sterile neutrinos. We reexamine this model and find that the sterile neutrinos can be…

高能物理 - 唯象学 · 物理学 2008-11-26 Scott Dodelson , Lawrence M. Widrow

In addition to the problem of galaxy formation, one of the greatest open questions of cosmology is represented by the existence of an asymmetry between matter and antimatter in the baryonic component of the Universe. We believe that a net…

天体物理学 · 物理学 2010-12-09 M. Lattanzi , R. Ruffini , G. Vereshchagin

The simplest possibility to explain the baryon asymmetry of the Universe is to assume that radiation is created asymmetrically between baryons and anti-baryons after the inflation. We propose a new mechanism of this kind where CP-violating…

高能物理 - 唯象学 · 物理学 2020-04-01 Shintaro Eijima , Ryuichiro Kitano , Wen Yin

Production of single neutrinos as well as neutrino-antineutrino pairs by photons interacting with pseudo Nambu-Goldstone bosons is studied within the Standard Model. The corresponding cross sections are found analytically. The energy loss…

高能物理 - 唯象学 · 物理学 2013-10-22 I. Alikhanov

We propose that the dark matter of our Universe could be sterile neutrinos which reside within the twin sector of a mirror twin Higgs model. In our scenario, these particles are produced through a version of the Dodelson-Widrow mechanism…

高能物理 - 唯象学 · 物理学 2024-03-20 Ian Holst , Dan Hooper , Gordan Krnjaic , Deheng Song

The back reaction effect of the neutrino field at finite temperature in the background of the static Einstein universe is investigated. A relationship between the temperature of the universe and its radius is found. As in the previously…

广义相对论与量子宇宙学 · 物理学 2009-11-07 M. B. Altaie

Recently, a new theory based on superluminal tunnelling has been proposed to explain the transition of highly energetic neutrinos propagating in matter to tachyonic states. In this work, we determine the possible mechanisms that lead…

综合物理 · 物理学 2020-02-07 Luca Nanni

We demonstrate for the first time that three sterile neutrinos alone can simultaneously explain neutrino oscillations, the observed dark matter and the baryon asymmetry of the Universe without new physics above the Fermi scale. The key new…

高能物理 - 唯象学 · 物理学 2013-03-01 Laurent Canetti , Marco Drewes , Mikhail Shaposhnikov

We calculate the incoherent resonant and non-resonant scattering production of sterile neutrinos in the early universe. We find ranges of sterile neutrino masses, vacuum mixing angles, and initial lepton numbers which allow these species to…

天体物理学 · 物理学 2009-11-06 K. Abazajian , G. M. Fuller , M. Patel

Neutrino properties can play a crucial role in determining the matter-antimatter asymmetry of the universe if thermal leptogenesis is the correct solution to the baryogenesis problem. Owing to this, the study of neutrino models goes beyond…

高能物理 - 唯象学 · 物理学 2009-01-12 Sandy S. C. Law

A new concept is proposed to solve the solar neutrino problem, that is based on a hypothesis about the existence of a new interaction of electron neutrinos with nucleons mediated by massless pseudoscalar bosons. At every collision of a…

高能物理 - 唯象学 · 物理学 2019-12-24 L. M. Slad

Neutrino--antineutrino ($\nu\bar\nu$) pair production is one of the main processes responsible for the energy loss of stars. Apart from the collision of two ($\gamma\gamma\to\nu\bar\nu$) or three ($\gamma\gamma\gamma\to\nu\bar\nu$) real…

高能物理 - 唯象学 · 物理学 2023-08-29 Naser Ahmadiniaz , Rashid Shaisultanov , Ralf Schützhold

Explicit expressions for the differential and total rates and emissivities of neutrino pairs from the photo-neutrino process $e^\pm + \gamma \to e^\pm + \nu + \bar\nu$ in hot and dense matter are derived. Full information about the emitted…

天体物理学 · 物理学 2009-11-10 Sharada Iyer Dutta , Sasa Ratkovic , Madappa Prakash

Present limits on neutrino masses are briefly reviewed, along with cosmological and astrophysical hints from dark matter, solar and atmospheric neutrino observations that suggest neutrino masses. These would imply many possible new…

高能物理 - 唯象学 · 物理学 2009-09-25 JosÉ W. F. Valle

In many realizations of leptogenesis, heavy right-handed neutrinos play the main role in the generation of an imbalance between matter and antimatter in the early Universe. Hence, it is relevant to address quantitatively their dynamics in a…

Observational manifestations of possible breaking of spin-statistics relation for neutrinos are considered. It is argued that bosonic neutrinos may form cosmological cold dark matter, improve agreement of BBN predictions with observations,…

高能物理 - 唯象学 · 物理学 2007-05-23 A. D. Dolgov

Several models of quantum open systems are known at present to violate, according to principles of the standard quantum theory of open systems, the second law of thermodynamics. Here, a new and rather trivial model of another type is…

统计力学 · 物理学 2007-05-23 V. Capek

Parity and time reversal are obvious and plausible candidates for fundamental symmetries of nature. Hypothesising that these symmetries exist implies the existence of a new form of matter, called mirror matter. The mirror matter theory (or…

天体物理学 · 物理学 2008-11-26 R. Foot

Special relativity allows massless particles to have states of different integer (or half-integer) helicities that mix under boosts, much like the spin-states of a massive particle. Such massless particles are known as continuous spin…

高能物理 - 唯象学 · 物理学 2025-06-26 Philip Schuster , Gowri Sundaresan , Natalia Toro

Left-Right symmetric theories solve the strong CP problem and explain the small Higgs quartic coupling at high energy scales via the Higgs Parity mechanism, which forces the Higgs quartic coupling to vanish at the Left-Right symmetry…

高能物理 - 唯象学 · 物理学 2021-05-19 David Dunsky , Lawrence J. Hall , Keisuke Harigaya