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Three-generation MSW effect in curved spacetime is studied and a brief discussion on the gravitational correction to the neutrino self-energy is given. The modified mixing parameters and corresponding conversion probabilities of neutrinos…

高能物理 - 唯象学 · 物理学 2016-09-14 Yu-Hao Zhang , Xue-Qian Li

Various theoretical arguments motivate an expectation of a phase transition in matter at extreme densities above nuclear density, accompanied by hopes that gravitational wave observations may reveal the properties of such a transition.…

广义相对论与量子宇宙学 · 物理学 2021-06-09 Steven L. Liebling , Carlos Palenzuela , Luis Lehner

We study Dirac neutrinos propagating in rotating background matter. First we derive the Dirac equation for a single massive neutrino in the noninertial frame, where matter is at rest. This equation is written in the effective curved…

高能物理 - 唯象学 · 物理学 2015-08-11 Maxim Dvornikov

We provide details and present additional results on the numerical study of the gravitational-wave emission from the collapse of neutron stars to rotating black holes in three dimensions. More specifically, we concentrate on the advantages…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Luca Baiotti , Ian Hawke , Luciano Rezzolla

New methods are proposed with the goal to determine absolute neutrino masses from the simultaneous observation of the bursts of neutrinos and gravitational waves emitted during a stellar collapse. It is shown that the neutronization…

高能物理 - 唯象学 · 物理学 2009-11-07 N. Arnaud , M. Barsuglia , M. A. Bizouard , F. Cavalier , M. Davier , P. Hello , T. Pradier

The frequencies of quasi-periodic oscillations around neutron stars are believed to be related to characteristic frequencies in the gravitational fields of the compact objects. In different variability models, these include the Keplerian,…

天体物理学 · 物理学 2007-05-23 Simon DeDeo , Dimitrios Psaltis

We explore the impact of corrections to the propagation on the waveforms of gravitationally lensed gravitational waves under the geometrical optics approximation, focusing on both uniform cosmological modifications and local modifications…

广义相对论与量子宇宙学 · 物理学 2025-03-03 Hiroki Takeda , Takahiro Tanaka

It is well known that when the distance $t$ traveled by neutrinos in matter is short, matter effects in oscillations of neutrino flavour are small and decrease with decreasing $t$ more rapidly than the oscillations effects themselves. We…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov

An introduction to various topics in neutrino astrophysics is given for students with little prior exposure to this field. We explain neutrino production and propagation in stars, neutrino oscillations, and experimental searches for this…

高能物理 - 唯象学 · 物理学 2007-05-23 G. G. Raffelt , W. Rodejohann

Accelerated expansion of the Universe prompted searches of modified gravity theory beyond general relativity, instead of adding a mysterious dark energy component with exotic physical properties. One such alternative gravity approach is…

广义相对论与量子宇宙学 · 物理学 2024-06-11 Sreekanth Harikumar , Laur Järv , Margus Saal , Aneta Wojnar , Marek Biesiada

Do neutrinos have nonzero masses? If they do, then these masses are very tiny, and can be sought only in very sensitive experiments. The most sensitive of these search for neutrino oscillation, a quantum interference effect which requires…

高能物理 - 唯象学 · 物理学 2017-08-23 Boris Kayser

We demonstrate that there exists a new mechanism for dissipating the energy of stellar oscillations. For neutron stars, in particular, we show that the mechanical energy of density perturbations is not only dissipated to heat via bulk…

太阳与恒星天体物理 · 物理学 2010-06-24 Basil A. Sa'd , Jürgen Schaffner-Bielich

Within the standard effective field theory of General Relativity, we show that the speed of gravitational waves deviates, ever so slightly, from luminality on cosmological and other spontaneously Lorentz-breaking backgrounds. This effect…

高能物理 - 理论 · 物理学 2020-03-25 Claudia de Rham , Andrew J. Tolley

We study the neutrino oscillation problem in the framework of the wave packet formalism. The neutrino state is described by a packet located initially in a region S (source) and detected in another region D at a distance R from S. We…

高能物理 - 唯象学 · 物理学 2008-11-26 Mikhail I. Shirokov , Vadim A. Naumov

Quantum coherence can significantly increase the strength of the forward scattering of neutrinos propagating through the Earth and interacting with matter. The index of refraction of the neutrinos propagating in a medium and hence their…

高能物理 - 唯象学 · 物理学 2015-05-30 Ram Brustein , Dmitri Semikoz

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

Astrophysical implications of gravitational microlensing of gravitational waves emitted by rotating neutron stars (NSs) are investigated. In particular, attention is focused on the following situations: i) NSs in the galactic bulge lensed…

天体物理学 · 物理学 2009-10-31 F. De Paolis , G. Ingrosso , A. A. Nucita

We study gravitational lensing of gravitational waves taking into account the spin of a graviton coupled with a dragged spacetime made by a rotating object. We decompose the phase of gravitational waves into helicity-dependent and…

广义相对论与量子宇宙学 · 物理学 2024-12-09 Kei-ichiro Kubota , Shun Arai , Shinji Mukohyama

We introduce a model in which the genesis of dark matter (DM) and neutrino masses is associated with a first order phase transition of a scalar singlet field. During the phase transition a source right-handed neutrino (RHN) acquires a…

高能物理 - 唯象学 · 物理学 2020-11-17 Pasquale Di Bari , Danny Marfatia , Ye-Ling Zhou

Because the propagation of neutrinos is affected by the presence of Earth matter, it opens new possibilities to probe the Earth's interior. Different approaches range from techniques based upon the interaction of high energy (above TeV)…

地球物理 · 物理学 2008-11-26 Walter Winter
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