Results 41 to 50 of about 74,471 (120)
Turbulence and supernova neutrinos
As neutrinos propagate from the neutrinosphere through the mantle of a core-collapse supernova they will pass through regions of turbulence. The turbulence leads to stochastic neutrino flavor mixing thus leaving fingerprints in the Galactic supernova ...
Kneller, James P.
core +1 more source
Gravitational lensing of supernova neutrinos [PDF]
The black hole at the center of the galaxy is a powerful lens for supernova neutrinos. In the very special circumstance of a supernova near the extended line of sight from Earth to the galactic center, lensing could dramatically enhance the neutrino flux
Quigg, Chris +3 more
core +1 more source
We examine the weak cosmic censorship conjecture (WCCC) violation by throwing a charged and rotating test particle into a Kerr–Newman–modified gravity black hole (KN–MOG BH). The result depends on several factors, such as the relative sign of the particle’s charge and its direction of rotation with respect to black hole (BH).
Waqar Ahmad +2 more
wiley +1 more source
Orientadores: Marcelo Moraes Guzzo, Pedro Cunha de HolandaTese (doutorado) - Universidade Estadual de Campinas, Instituto de Física Gleb WataghinResumo: Neutrinos de supernova são ferramentas fundamentais, tanto para se entender o mecanismo de explosão ...
Torres, Fernando Rossi, 1982-
core
Supernova Neutrinos: Challenges and Opportunities
Neutrinos are crucial ingredients for supernova explosions, and come to us bearing important particle physics and astrophysics information. Current and upcoming neutrino detectors are poised to detect these neutrinos, either as a diffuse background or ...
Dasgupta, Basudeb +1 more
core +1 more source
Analytical Description of the Distributions of Primary and Secondary Cosmogenic Particles
In this work, we present an analytical description of the energy distributions of primary and secondary cosmogenic particles on Earth in terms of parameters having clear physical meaning. A modified power law is assumed for energy distributions, incorporating terms such as energy loss/decay, which are effective at low energies, and a source term, which
Shvetaank Tripathi +2 more
wiley +1 more source
KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS [PDF]
In the late stages of nuclear burning for massive stars (M > 8 M⊙), the production of neutrino–antineutrino pairs through various processes becomes the dominant stellar cooling mechanism.
Enomoto, S +46 more
core +5 more sources
Abstract Dielectric anisotropy in ice alters the propagation of polarized radio waves, so polarimetric radar sounding can be used to survey anisotropic properties of ice masses. Ice anisotropy is either intrinsic, associated with ice‐crystal orientation fabric (COF), or extrinsic, associated with material heterogeneity, such as bubbles, fractures, and ...
Benjamin H. Hills +30 more
wiley +1 more source
Neutrinos are pivotal signals in multimessenger observations of supernovae (SNe). Recent advancements in the analysis method of supernova (SN) neutrinos, especially in quantitative analysis, have significantly broadened scientific possibilities.
Yudai Suwa +9 more
doaj +1 more source
Two Micron‐Size Dark Dimensions
Abstract Two extra dimensions of micron scale might simultaneously address the gauge and cosmological hierarchy problems. In this paper various observational bounds in scenarios with one and two large extra dimensions are examined, to see if they are compatible with the micron scale.
Luis A. Anchordoqui +2 more
wiley +1 more source

