Results 101 to 110 of about 155,831 (295)

Probing the Origins of Neutrino Mass with Supernova Data

, 2005
We study type II supernova signatures of neutrino mass generation via symmetry breaking at a scale in the range from keV to MeV. The scalar responsible for symmetry breaking can be thermalized in the supernova core and restore the symmetry. The neutrinos
Davoudiasl, Hooman, Huber, Patrick
core   +1 more source

Electron Neutrino Mass Measurement by Supernova Neutrino Bursts and Implications on Hot Dark Matter [PDF]

, 1998
We present a new strategy for measuring the electron neutrino mass ($\mnue$) by future detection of a Galactic supernova in large underground detectors such as the Super-Kamiokande (SK).
A. Burrows, A. S. Joshipura, A. Yu. Smirnov, D. Caldwell, D. Caldwell, G. I. Zatsepin, G. I. Zatsepin, G. T. Ewan, J. R. Primack, J. R. Wilson, K. Langanke, K. Nakamura, R. Mayle, S. T. Petcov, T. J. Loredo, T. K. Gaisser, Tomonori Totani, Y. Totsuka   +17 more
core   +2 more sources

Spectrum of supernova neutrinos in ultra-pure scintillators [PDF]

, 2014
There is a great interest in measuring the non-electronic component of neutrinos from core collapse supernovae by observing, for the first time, also neutral-current reactions.
C. Lujan-Peschard, G. Pagliaroli, F. Vissani   +2 more
semanticscholar   +1 more source

Likelihood for supernova neutrino analyses [PDF]

Physical Review D, 2009
7 pages, 2 figures.
Ianni A, Pagliaroli G, Strumia A, Torres FR, VILLANTE, FRANCESCO LORENZO, Vissani F.   +5 more
openaire   +3 more sources

Supernova neutrinos and the turbulence power spectrum: point source statistics

, 2015
The neutrinos emitted from the proto-neutron star created in a core-collapse supernova must run through a significant amount of turbulence before exiting the star.
Kabadi, Neel V., Kneller, James P.
core   +1 more source

Heavy Elements and Electromagnetic Transients from Neutron Star Mergers

Annalen der Physik, Volume 536, Issue 2, February 2024.
Astro‐(physics) has made major leaps forward through the combined information provided by both gravitational waves and electromagnetic emission from the first detected neutron star merger event. This review provides an up‐to‐date overview of today's understanding of neutron star mergers and their electromagnetic emission and it discusses possible ...
Stephan Rosswog, Oleg Korobkin
wiley   +1 more source

Mass varying neutrinos in supernovae [PDF]

Physical Review D, 2011
8 pages, 5 ...
Rossi-Torres, F., Guzzo, M. M., De Holanda, P. C., Peres, O. L.G.   +3 more
openaire   +4 more sources

Observing Supernova Neutrino Light Curves with Super-Kamiokande. V. Distance Estimation with Neutrinos

The Astrophysical Journal
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, Akira Harada, Masamitsu Mori, Ken’ichiro Nakazato, Ryuichiro Akaho, Masayuki Harada, Yusuke Koshio, Fumi Nakanishi, Kohsuke Sumiyoshi, Roger A. Wendell   +9 more
doaj   +1 more source

Convoluted ν-Signals on 114Cd Isotope from Astrophysical and Laboratory Neutrino Sources

Advances in High Energy Physics, 2015
At first, we evaluate scattering cross sections of low, and intermediate-energy neutrinos scattered off the 114 Cd isotope, the most abundant Cd isotope present also in the COBRA detector (CdTe and CdZnTe materials) which aims to search for double beta ...
Vaitsa Tsakstara
doaj   +1 more source

Supernova neutrino detection on earth [PDF]

Chinese Physics C, 2010
5 pages, 2 ...
Huang Ming-Yang, Young Bing-Lin, Young Bing-Lin, Guo Xin-Heng   +3 more
openaire   +4 more sources