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相关论文: Neutrinos as a probe of curvature

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The present paper has developed an integro-differential equation to propagate cosmological gravitation waves in matter-dominated era in accounting for the presence of free streaming neutrinos as a traceless transverse tensor part of the…

广义相对论与量子宇宙学 · 物理学 2016-08-08 Jafar Khodagholizadeh , Amir H. Abbassi , Ali A. Asgari

This paper explains the significance of neutrino mass in the cosmic progression from the radiation-dominated phase to matter and subsequently to the dark energy-dominated era. We have put a constraint on the total mass of neutrinos by…

广义相对论与量子宇宙学 · 物理学 2023-12-11 Muhammad Yarahmadi , Amin Salehi

As the increasing of neutrino energy or matter density, the neutrino oscillation in matter may undergo "vacuum-dominated", "resonance" and "matter-dominated" three different stages successively. Neutrinos endure very different matter…

高能物理 - 唯象学 · 物理学 2020-02-26 Shu Luo

We explore the dynamics of neutrinos in a vacuum dominated cosmology. First we show that such a geometry will induce a phase change in the eigenstates of a massive neutrino and we calculate the phase change. We also calculate the delay in…

天体物理学 · 物理学 2007-05-23 Manasse R. Mbonye

We investigate the implications of decoherence induced by quantum spacetime properties on neutrino oscillation phenomena. We develop a general formalism where the evolution of neutrinos is governed by a Lindblad-type equation and we compute…

高能物理 - 唯象学 · 物理学 2024-05-22 Vittorio D'Esposito , Giulia Gubitosi

We obtain the equation governing the evolution of the cosmological gravitational-wave background, accounting for the presence of cosmic neutrinos, up to second order in perturbation theory. In particular, we focus on the epoch during…

天体物理学 · 物理学 2009-02-23 A. Mangilli , N. Bartolo , S. Matarrese , A. Riotto

We derive an integro-differential equation for propagation of cosmological gravitation waves in spatially closed cosmology whereas the traceless transverse tensor part of the anisotropic stress tensor is free streaming neutrinos (including…

宇宙学与河外天体物理 · 物理学 2014-09-25 Jafar Khodagholizadeh , Amir H. Abbassi , Ali A. Asgari

An analytic formula is given for the traceless transverse part of the anisotropic stress tensor due to free streaming neutrinos, and used to derive an integro-differential equation for the propagation of cosmological gravitational waves.…

天体物理学 · 物理学 2009-11-07 Steven Weinberg

The damping effect of the free-streaming neutrinos on the second order gravitational waves is investigated in detail. We solve the Boltzmann equation and give the anisotropic stress induced by neutrinos to second order. The first order…

宇宙学与河外天体物理 · 物理学 2022-09-08 Xukun Zhang , Jing-Zhi Zhou , Zhe Chang

The objective of this study is to verify the consistency of the prescription of alternative minimum coupling (connection) proposed by the Teleparallel Equivalent to General Relativity (TEGR) for the Dirac equation. With this aim, we studied…

广义相对论与量子宇宙学 · 物理学 2009-12-22 A. A. Sousa , D. M. Oliveira , R. B. Pereira

Space-time localization diagrams ``unlock" subtle aspects of $\nu$ oscillations such as coherence and entanglement. Observability of propagation decoherence in oscillating neutrino state is discussed. The sizes of WPs of reactor and source…

高能物理 - 唯象学 · 物理学 2022-12-21 Alexei Y Smirnov

Using the Einstein-Cartan-Dirac theory, we study the effect of torsion on neutrino oscillation. We see that torsion cannot induce neutrino oscillation, but affects it whenever oscillation exists for other reasons. We show that the torsion…

广义相对论与量子宇宙学 · 物理学 2009-10-31 M. alimohammadi , A. Shariati

This paper investigates the influence of non-commutative geometry on various aspects of neutrino behavior in curved spacetime. Adopting a Schwarzschild-like black hole solution with Lorentzian mass deformation induced by non-commutativity,…

广义相对论与量子宇宙学 · 物理学 2025-04-08 A. A. Araújo Filho , N. Heidari , Yuxuan Shi

The gravitational neutrino oscillation problem is studied by considering the Dirac Hamiltonian in a Riemann-Cartan space-time and calculating the dynamical phase. Torsion contributions which depend on the spin direction of the mass…

广义相对论与量子宇宙学 · 物理学 2010-12-23 M. Adak , T. Dereli , L. H. Ryder

We discuss neutrino oscillations in curved spacetime. Our heuristic approach can accomodate matter effects and gravitational contributions to neutrino spin precession in the presence of a magnetic field. By way of illustration, we perform…

高能物理 - 唯象学 · 物理学 2009-10-30 Christian Y. Cardall , George M. Fuller

The neutrino oscillations in the field of a rotating deformed mass is investigated. The phase shift is evaluated in the case of weak field limit, slow rotation and small deformation. To this aim the Hartle-Thorne metric is used, which is an…

广义相对论与量子宇宙学 · 物理学 2015-06-04 Andrea Geralico , Orlando Luongo

We propose a modified Dirac equation for a massive neutrino moving in the presence of the background matter. The effects of the charged and neutral-current interactions with the matter as well as the matter motion and polarization are…

高能物理 - 唯象学 · 物理学 2021-01-19 Alexander Studenikin , Alexei Ternov

In this work, we derive novel constraints on scalar-tensor theories from neutrino physics. Spatial variations of the background scalar field effectively generate density and position-dependent Standard Model masses, including neutrinos.…

高能物理 - 唯象学 · 物理学 2025-12-17 Arturo de Giorgi , Ivan Martinez Soler , Sergio Sevillano Muñoz

Most of our knowledge of the universe has been obtained from the anisotropy spectrum of the cosmic microwave background and observations of large-scale structures. During the history of the Universe, neutrinos from the early Universe evolve…

广义相对论与量子宇宙学 · 物理学 2023-10-31 Muhammad Yarahmadi , Amin Salehi

We study neutrino oscillations in a medium of dark matter which generalizes the standard matter effect. A general formula is derived to describe the effect of various mediums and their mediators to neutrinos. Neutrinos and anti-neutrinos…

高能物理 - 唯象学 · 物理学 2019-10-08 Ki-Young Choi , Eung Jin Chun , Jongkuk Kim
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