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We study inelastic neutrino scattering off hot nuclei for temperatures relevant under supernova conditions. The method we use is based on the quasiparticle random phase approximation extended to finite temperatures within the thermo field…

核理论 · 物理学 2014-03-18 Alan A. Dzhioev , A. I. Vdovin , J. Wambach , V. Yu. Ponomarev

In supersymmetric models with lepton-number violation, hence also R-parity violation, it is easy to have realistic neutrino masses, but then leptogenesis becomes difficult to achieve. After explaining the general problems involved, we study…

高能物理 - 唯象学 · 物理学 2009-10-31 Thomas Hambye , Ernest Ma , Utpal Sarkar

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

We review the collider phenomenology of neutrino physics and the synergetic aspects at energy, intensity and cosmic frontiers to test the new physics behind the neutrino mass mechanism. In particular, we focus on seesaw models within the…

高能物理 - 唯象学 · 物理学 2015-08-05 Frank F. Deppisch , P. S. Bhupal Dev , Apostolos Pilaftsis

Thermal leptogenesis requires the reheating temperature $T_R \gsim 3\times 10^{9}$ GeV, which contradicts a recently obtained constraint on the reheating temperature, $T_R \lsim 10^6$ GeV, for the gravitino mass of 100 GeV-10 TeV. This…

高能物理 - 唯象学 · 物理学 2015-06-25 M. Fujii , M. Ibe , T. Yanagida

We calculate the differential scattering rate for thermal neutrinos in a hot and dilute gas of interacting neutrons using linear response theory. The dynamical structure factors for density and spin fluctuations of the strongly interacting…

核理论 · 物理学 2018-08-08 Paulo F. Bedaque , Sanjay Reddy , Srimoyee Sen , Neill C. Warrington

The R-symmetry formalism is applied for the supersymmetric economical SU(3)_C X SU(3)_L X U(1)_X (3-3-1) model. The generalization of the minimal supersymmetric standard model relation among R-parity, spin and matter parity is derived, and…

高能物理 - 唯象学 · 物理学 2011-10-13 P. V. Dong , D. T. Huong , M. C. Rodriguez , H. N. Long

By extending the lepton sector of standard model to include one sterile neutrino and two sets of new Higgs doublets and right-handed neutrinos, denoted by $(\eta_1, N_1, N_3)$ and $(\eta_2, N_2, N_4)$, with two $Z_2$ symmetries, the puzzles…

高能物理 - 唯象学 · 物理学 2009-05-26 Chuan-Hung Chen

With the standard electroweak interactions, the lowest-order coherent forward scattering amplitudes of neutrinos in a CP symmetric medium (such as the early universe) are zero, and the index of refraction of a propagating neutrino can only…

高能物理 - 唯象学 · 物理学 2009-12-30 Paul Langacker , Jiang Liu

We consider a minimal extension of the Standard Model with one singlet neutrino per generation that can realize resonant leptogenesis at the electroweak scale. In particular, the baryon asymmetry in the Universe can be created by resonant…

高能物理 - 唯象学 · 物理学 2009-11-10 Apostolos Pilaftsis

We demonstrate a common origin for high-scale leptogenesis and three-loop neutrino mass generation. Specifically we extend the standard model by two real singlet scalars, two singly charged scalars carrying different lepton numbers and two…

高能物理 - 唯象学 · 物理学 2017-05-24 Pei-Hong Gu

We report measurements of resonant low-energy electron attachment to O\(_2\) molecular impurities in neon gas in the temperature range \(46.5\,\mbox{K}\le T\le 101\,\mbox{K}\). The reduced attachment frequency \(\nu_A/N\) shows a well…

等离子体物理 · 物理学 2020-04-22 A. F. Borghesani

Upper bounds on the CP asymmetry relevant for leptogenesis are reexamined and found weaker than in previous literature, both for hierarchical and for quasi-degenerate right-handed neutrinos. Successful leptogenesis implies the usual lower…

高能物理 - 唯象学 · 物理学 2009-10-09 Thomas Hambye , Yin Lin , Alessio Notari , Michele Papucci , Alessandro Strumia

We discuss the bulk viscosity of hot and dense $npe\mu$ matter arising from weak-interaction direct Urca processes. We consider two regimes of interest: (a) the neutrino-transparent regime with $T\leq T_{\rm tr}$ ($T_{\rm tr}\simeq 5\div…

高能天体物理现象 · 物理学 2022-09-13 Mark Alford , Arus Harutyunyan , Armen Sedrakian

Under the assumption of hierarchical right-handed neutrino masses, masses of right-handed neutrinos must be larger than $10^8$ GeV in the standard thermal leptogenesis scenario, while the mass can be reduced to around 5 TeV in a…

高能物理 - 唯象学 · 物理学 2013-08-15 Naoyuki Haba , Osamu Seto , Yuya Yamaguchi

We apply phase-space density considerations to obtain lower bounds on the mass of sterile neutrino as dark matter candidate. The bounds are different for non-resonant production, resonant production in the presence of lepton asymmetry and…

高能物理 - 唯象学 · 物理学 2009-12-04 D. Gorbunov , A. Khmelnitsky , V. Rubakov

We present a three-loop model of neutrino mass whose most-general Lagrangian possesses a softly-broken accidental $Z_2$ symmetry. In the limit that a single parameter vanishes, $\lambda\rightarrow0$, the $Z_2$ symmetry becomes exact and the…

高能物理 - 唯象学 · 物理学 2014-11-04 Amine Ahriche , Kristian L. McDonald , Salah Nasri

If the minimal standard model of particle interactions is extended to include a scalar triplet with lepton number $L=-2$ and a scalar doublet with $L=-1$, neutrino masses $m_\nu \sim \mu_{12}^4 v^2/M^5 \sim 10^{-2}$ eV is possible, where $v…

高能物理 - 唯象学 · 物理学 2009-11-07 Ernest Ma

We investigate nuclear pasta structures at high temperatures in the framework of relativistic mean field model with Thomas-Fermi approximation. Typical pasta structures (droplet, rod, slab, tube, and bubble) are obtained, which form various…

核理论 · 物理学 2022-09-28 Cheng-Jun Xia , Toshiki Maruyama , Nobutoshi Yasutake , Toshitaka Tatsumi

A brief analysis of the result of the Neutrino-4 experiment and the results of other experiments on the search for a sterile neutrino is presented. It is noted that a joint analysis of the results of the Neutrino-4 experiment and the data…

高能物理 - 唯象学 · 物理学 2023-02-23 A. P. Serebrov , R. M. Samoilov , M. E. Chaikovskii , O. M. Zherebtsov
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