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IceCube observed high-energy neutrino flux in the energy region from TeV to PeV. The decay of a massive long-lived particle in the early universe can be the origin of the IceCube neutrino events, which we call an "early decay scenario." In…

高能物理 - 唯象学 · 物理学 2016-10-05 Yohei Ema , Takeo Moroi

We study the possible structure of the neutrino mass matrix taking into consideration the solar and atmospheric neutrinos and the neutrinoless double beta decay. We emphasize on mass matrices with vanishing elements. There are only a very…

高能物理 - 唯象学 · 物理学 2017-08-23 H. V. Klapdor-Kleingrothaus , U. Sarkar

If there exist unstable but long-lived relics of the early universe, their decays could produce detectable fluxes of gamma rays and neutrinos. In this paper, we point out that the decays of superheavy particles, $m_{\chi} \gtrsim 10^{10} \,…

高能物理 - 唯象学 · 物理学 2025-02-19 Kim V. Berghaus , Dan Hooper , Emily R. Simon

New results, namely the independent determination of the deuterium abundance in several quasar absorption systems, and the complementary determination of the cosmological baryon density by observations of anisotropies in the cosmic…

天体物理学 · 物理学 2008-11-26 Kevork N. Abazajian

Future cosmological measurements should enable the sum of neutrino masses to be determined indirectly through their effects on the expansion rate of the Universe and the clustering of matter. We consider prospects for the gravitationally…

宇宙学与河外天体物理 · 物理学 2015-12-30 Rupert Allison , Paul Caucal , Erminia Calabrese , Joanna Dunkley , Thibaut Louis

Neutrino decay in the minimal seesaw model containing three right handed neutrinos and a complex $SU(2)\times U(1)$ singlet Higgs in addition to the standard model fields is considered. A global horizontal symmetry $U(1)_H$ is imposed,…

高能物理 - 唯象学 · 物理学 2009-10-22 Anjans S. Joshipura , Saurabh D. Rindani

A decaying particle that dominates the energy density of the universe and then decays with a lifetime $\sim 10^{-1}$ sec into electromagnetically-interacting particles can heat the background electron neutrinos more than the $\mu$ and…

天体物理学 · 物理学 2007-05-23 Richard E. Leonard , Robert J. Scherrer

The neutrino produced in the pion decay reveals a new diffraction phenomenon due to many-body interactions in an intermediate time region when wave functions of the parent and daughters overlap. Because of diffraction, the probability to…

高能物理 - 唯象学 · 物理学 2012-11-28 Kenzo Ishikawa , Yutaka Tobita

Several non-threshold reactions which may be used to detect the cosmic neutrino background are presented. The corresponding cross sections are calculated analytically within the Standard Model. These reactions are sensitive not only to the…

宇宙学与河外天体物理 · 物理学 2014-07-31 I. Alikhanov

By requiring the lower limit for the lightest right-handed neutrino mass, obtained in the baryogenesis from leptogenesis scenario, and a Dirac neutrino mass matrix similar to the up-quark mass matrix we predict small values for the $\nu_e$…

高能物理 - 唯象学 · 物理学 2009-11-10 F. Buccella , D. Falcone

We study the nonresonant oscillations between left-handed electron neutrinos nu_e and nonthermalized sterile neutrinos nu_s in the early Universe plasma. The case when nu_s do not thermalize till 2 MeV and the oscillations become effective…

高能物理 - 唯象学 · 物理学 2011-02-24 D. P. Kirilova , M. V. Chizhov

The small-scale power spectrum of the cosmological matter distribution together with other cosmological data provides a sensitive measure of the hot dark matter fraction, leading to restrictive neutrino mass limits. We extend this argument…

高能物理 - 唯象学 · 物理学 2009-11-10 Steen Hannestad , Georg Raffelt

Neutrino oscillations in the early Universe prior to the epoch of primordial nucleosynthesis is studied by implementing real time non-equilibrium field theory methods. We focus on two flavors of Dirac neutrinos, however, the formulation is…

高能物理 - 唯象学 · 物理学 2009-11-11 C. M. Ho , D. Boyanovsky , H. J. de Vega

A massive particle decaying into neutrinos in the early Universe is known to be less constrained than if it was decaying into other standard model particles. However, even if the decay proceeds into neutrinos, the latter still inevitably…

高能物理 - 唯象学 · 物理学 2022-06-01 Thomas Hambye , Marco Hufnagel , Matteo Lucca

A lower bound on the light neutrino mass $m_\nu$ is derived in the framework of a geometrical interpretation of quantum mechanics. Using this model and the time of flight delay data for neutrinos coming from SN1987A, we find that the…

广义相对论与量子宇宙学 · 物理学 2009-11-11 G. Lambiase , G. Papini , R. Punzi , G. Scarpetta

Due to sphaleron processes in the high-temperature symmetric phase of the standard model the cosmological baryon asymmetry is related to neutrino properties. For hierarchical neutrino masses, with $B-L$ broken at the unification scale…

高能物理 - 唯象学 · 物理学 2008-11-26 W. Buchmüller , M. Plümacher

Assuming that neutrinos are spacelike (tachyonic) fermions, we calculate width for the kinematically allowed, lepton number conserving, three-body decay $\nu_{\alpha}\rightarrow \nu_{\alpha} \; \nu_{\beta} \bar{\nu}_{\beta}$ in the Standard…

高能物理 - 唯象学 · 物理学 2023-10-05 Jakub Rembielinski , Jacek Ciborowski

The quantum decay of a relativistic scalar field from a metastable state ("false vacuum decay") is a fundamental idea in quantum field theory and cosmology. This occurs via local formation of bubbles of true vacuum with their subsequent…

Several anomalies in neutrino oscillation experiments point to the existence of a $\sim 1\,$eV sterile neutrino $\nu_s$ mixing with $\nu_e$ at the level of $U_{e4}\cong 0.1$, but such a neutrino is strongly disfavored by constraints on…

高能物理 - 唯象学 · 物理学 2020-01-15 James M. Cline

In this paper we consider the coherence properties of neutrinos produced by the decays of pions in conventional neutrino beams. Using a multi-particle density matrix formalism we derive the oscillation probability for neutrinos emitted by a…

高能物理 - 唯象学 · 物理学 2015-03-11 B. J. P. Jones