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相关论文: Neutrino oscillations and supernovae

200 篇论文

The time dependent neutrino oscillation signals due to the passage of a shock wave through the supernovae are analyzed for the case of three active neutrinos and also for the case that there are two additional sterile neutrinos. It is shown…

高能物理 - 唯象学 · 物理学 2008-11-26 Sandhya Choubey , N. P. Harries , G. G. Ross

We all know that in the dense anisotropic interior of the star, neutrino-neutrino forward-scattering can lead to fast collective neutrino oscillations, which has striking consequences on flavor dependent neutrino emission and can be crucial…

高能物理 - 唯象学 · 物理学 2021-01-06 Soumya Bhattacharyya

We have explored the impact of sterile neutrino dark matter on core-collapse supernova explosions. We have included oscillations between electron neutrinos or mixed $\mu,\tau$ neutrinos and right-handed sterile neutrinos into a supernova…

高能天体物理现象 · 物理学 2016-04-11 Grant J. Mathews , MacKenzie Warren , Jun Hidaka , Toshitaka Kajino

The neutrino propagation and oscillations in various gravitational fields are studied. First, we consider the neutrino scattering off a black hole accounting for the neutrino spin precession. Then, we study the evolution of flavor neutrinos…

高能物理 - 唯象学 · 物理学 2022-08-12 Maxim Dvornikov

We discuss the possibility of sterile neutrinos taking shortcuts in extra dimensions, and the consequences for neutrino oscillations. This effect influences the active-sterile neutrino mixing and provides a possibility to accommodate the…

高能物理 - 唯象学 · 物理学 2008-11-26 Heinrich Päs , Sandip Pakvasa , Thomas J. Weiler

The observation of Earth matter effects in the spectrum of neutrinos coming from a next galactic core-collapse supernova (CCSN) could, in principle, reveal if neutrino mass ordering is normal or inverted. One of the possible ways to…

高能物理 - 唯象学 · 物理学 2022-01-12 Edwin A. Delgado , Hiroshi Nunokawa , Alexander A. Quiroga

In this lecture we review some of the basic properties of neutrinos, in particular their mass and the oscillation behavior. First we discuss how to describe the neutrino mass. Then, under the assumption that neutrinos are massive and mixed,…

高能物理 - 唯象学 · 物理学 2007-05-23 C. W. Kim

In this essay, we introduce a new effect of gravitationally induced quantum mechanical phases in neutrino oscillations. These phases arise from an hitherto unexplored interplay of gravitation and the principle of the linear superposition of…

广义相对论与量子宇宙学 · 物理学 2023-04-19 D. V. Ahluwalia , C. Burgard

Neutrinos are neutral, spin-$\frac{1}{2}$ particles which undergo only weak interactions. The experimentally observed phenomenon of neutrino oscillation establishes the fact that neutrinos are massive and there is mixing between different…

高能物理 - 唯象学 · 物理学 2016-03-16 Monojit Ghosh

The wind driven by the intense neutrino emission from a protoneutron star (PNS) is an important site for producing nuclei heavier than the Fe group. Because of certain features in the neutrino angular distributions, the so-called fast…

高能天体物理现象 · 物理学 2020-12-21 Zewei Xiong , Andre Sieverding , Manibrata Sen , Yong-Zhong Qian

Some of the hot topics in neutrino physics are discussed, with particular emphasis on neutrino oscillations. After proposing credibility criteria for assessing various claimed effects, particular stress is laid on the solar neutrino…

高能物理 - 唯象学 · 物理学 2007-05-23 John Ellis

I discuss the implications of neutrino oscillations for neutrino mass patterns and mass matrices, and for neutrinoless double beta decay. I then go on to discuss the implications for cosmological relic density and dark matter, the galaxy…

高能物理 - 唯象学 · 物理学 2008-11-26 S. F. King

We point out that solar neutrino oscillations with large mixing angle as evidenced in current solar neutrino data have a strong impact on strategies for diagnosing collapse-driven supernova (SN) through neutrino observations. Such…

高能物理 - 唯象学 · 物理学 2009-09-17 H. Minakata , H. Nunokawa , R. Tomas , J. W. F. Valle

A brief overview of selected topics in the theory and phenomenology of neutrino oscillations is given. These include: oscillations in vacuum and in matter; phenomenology of 3-flavour neutrino oscillations and effective 2-flavour…

高能物理 - 唯象学 · 物理学 2007-05-23 E. Kh. Akhmedov

With myriads of detection events from a prospective Galactic core-collapse supernova, current and future neutrino detectors will be able to sample detailed, time-dependent neutrino fluxes and spectra. This offers enormous possibilities for…

高能天体物理现象 · 物理学 2019-09-04 B. Müller

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

Neutrinos play an important role in core-collapse supernova events since they are a key piece to understand the explosion mechanisms. The analysis of the neutrino fluxes can bring answers to neutrino's related problems e.g.: mass hierarchy,…

高能物理 - 唯象学 · 物理学 2022-05-11 M. M. Saez , M. E. Mosquera , O. Civitarese

Recently, stellar collapse involving black hole formation from massive stars is suggested to emit enormous fluxes of neutrinos on par with ordinary core-collapse supernovae. We investigate their detectability for the currently operating…

天体物理学 · 物理学 2014-11-18 Ken'ichiro Nakazato , Kohsuke Sumiyoshi , Hideyuki Suzuki , Shoichi Yamada

Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore,…

高能物理 - 唯象学 · 物理学 2016-12-07 Charles J. Stapleford , Daavid J. Väänänen , James P. Kneller , Gail C. McLaughlin , Brandon T. Shapiro

The inclusion of massive neutrinos affects the cross sections involved in the formation of heavy nuclei, modifying their abundances. Rapid neutron capture processes (r-process) are often associated with explosive events such as…

高能物理 - 唯象学 · 物理学 2018-09-10 M. M. Saez , M. E. Mosquera , O. Civitarese