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We consider the non-radiative two body decay of a neutrino to a daughter neutrino with degraded energy and a very light particle (Majoron). Ultrahigh energy neutrinos from an astrophysical source like a Gamma Ray Burst undergoing this decay…

天体物理学 · 物理学 2009-11-10 Nayantara Gupta , H. S. Mani

Light sterile neutrinos, $\nu_s$, are often introduced to explain an anomalous deficit in the electron antineutrino flux from nuclear reactors. If they exist, sterile neutrinos would also be produced in collapsing massive stars through the…

高能天体物理现象 · 物理学 2025-04-22 Kanji Mori , Tomoya Takiwaki , Kazunori Kohri , Hiroki Nagakura

We propose that future observations of supernova relic neutrinos (SRN) can be used to probe neutrino decay models. We focus on invisible (e.g. Majoron) decays, and work out the general solution of SRN kinetic equations in the presence of…

高能物理 - 唯象学 · 物理学 2007-05-23 G. L. Fogli , E. Lisi , A. Mirizzi , D. Montanino

If neutrinos are Dirac particles the existence of light right-handed neutrinos $\nu_{R}$ is implied. Those would contribute to the effective number of relativistic neutrino species $N_{{\rm eff}}$ in the early Universe. With pure standard…

高能物理 - 唯象学 · 物理学 2020-07-01 Xuheng Luo , Werner Rodejohann , Xun-Jie Xu

The thermodynamic equations of state for Majorana and Dirac fermions are quite different even in the limit of zero mass. The corresponding equations are derived from general principles, and then applied to neutrinos. The nature of the…

高能物理 - 唯象学 · 物理学 2007-05-23 Y. N. Srivastava , A. Widom , J. Swain

Heavy sterile-like neutrinos may be produced resonantly from the decay of pseudoscalar mesons and may decay into several different channels in a cascade $\Phi \rightarrow L^\alpha \nu_h;\nu_h\rightarrow \{X\}$. In general these are rare…

高能物理 - 唯象学 · 物理学 2014-10-14 Daniel Boyanovsky

The discovery of neutrino masses suggests the likely existence of gauge singlet fermions that participate in the neutrino mass generation via the seesaw mechanism. The masses of the corresponding degrees of freedom can range from well below…

高能物理 - 唯象学 · 物理学 2012-01-05 Alexander Kusenko

Recently, there has been a growing interest in extensions of the Standard Model in which naturally small Dirac neutrino masses arise due to existence of a symmetry which protects neutrino's Diracness. Motivated by this, we consider an…

高能物理 - 唯象学 · 物理学 2019-12-11 S. S. Correia , R. G. Felipe , F. R. Joaquim

We consider sterile neutrinos with rest masses ~0.2 GeV. Such sterile neutrinos could augment core collapse supernova shock energies by enhancing energy transport from the core to the vicinity of the shock front. The decay of these…

天体物理学 · 物理学 2010-04-28 George M. Fuller , Alexander Kusenko , Kalliopi Petraki

We formulate general conditions on $3\times 3$ neutrino mass matrices under which a degenerate pair of neutrinos at a high scale would split at low scale by radiative corrections involving only the standard model fields. This generalizes…

高能物理 - 唯象学 · 物理学 2009-10-31 Anjan S. Joshipura , Saurabh D. Rindani

Supernova cooling has long been used to constrain physics beyond the Standard Model, typically involving new mediators or dark matter (DM) particles that couple to nucleons or electrons. In this work, we show that the large density of…

高能物理 - 唯象学 · 物理学 2025-03-14 Christopher V. Cappiello , P. S. Bhupal Dev , Amol V. Patwardhan

The nature of neutrino masses and the matter-antimatter asymmetry of our universe are two of the most important open problems in particle physics today and are notoriously difficult to test with current technology. Dirac neutrinos offer a…

高能物理 - 唯象学 · 物理学 2023-08-10 Julian Heeck , Jan Heisig , Anil Thapa

There are now strong hints suggesting that neutrinos do have a mass after all. If they do have a mass, it would have to be tiny. Why is it so? Is it Dirac or Majorana? Can one build a model in which a teeny, tiny Dirac neutrino mass arises…

高能物理 - 唯象学 · 物理学 2009-10-31 P. Q. Hung

We investigate the muon neutrino event rate in km$^3$ neutrino telescopes due to a number of galactic supernova remnants expected on the basis of these objects' known $\gamma$-ray signals. We evaluate the potential of these neutrino signals…

天体物理学 · 物理学 2009-11-06 Roland M. Crocker , Fulvio Melia , Raymond R. Volkas

Large colliders are not sensitive to light neutrino masses and character, but they can produce new heavy neutrinos, allowing also for the determination of their Dirac or Majorana nature. We review the discovery limits at the next generation…

高能物理 - 唯象学 · 物理学 2008-11-26 F. del Aguila , J. A. Aguilar-Saavedra , R. Pittau

We investigate some consequences if neutrinoless double beta decays of nuclei are dominated by short range interactions. To illustrate our results, we assume that such decays proceed mainly through short range interactions involving…

高能物理 - 唯象学 · 物理学 2020-07-22 C. Q. Geng , J. N. Ng

We propose a new mechanism to generate minuscule active neutrino masses in a five-dimensional~(5d) spacetime of an interval without introducing $SU(2)_L$ singlet neutrinos. Under asymmetric boundary conditions on the two end points, a bulk…

高能物理 - 唯象学 · 物理学 2016-07-05 Yukihiro Fujimoto , K. Hasegawa , Tomoaki Nagasawa , Kenji Nishiwaki , Makoto Sakamoto , Kentaro Tatsumi

According to the "Black Box" theorem the experimental confirmation of neutrinoless double beta decay ($0 \nu 2 \beta$) would imply that at least one of the neutrinos is a Majorana particle. However, a null $0 \nu 2 \beta$ signal cannot…

高能物理 - 唯象学 · 物理学 2018-05-09 Martin Hirsch , Rahul Srivastava , José W. F. Valle

We present a scenario of neutrino masses and mixing angles. Each generation includes a sterile right handed neutrino in addition to the usual left handed one. We assume a hierarchy in their Dirac masses similar to, but much larger than the…

高能物理 - 唯象学 · 物理学 2016-08-24 D. Ring

In 2006, a simple extension of the Standard Model was proposed in which neutrinos obtain radiative Majorana masses at one-loop level from their couplings with dark matter, hence the term "scotogenic," from the Greek "scotos" meaning…

高能物理 - 唯象学 · 物理学 2013-05-30 Yasaman Farzan , Ernest Ma