Solar neutrinos as highlight of astroparticle physics [PDF]
arXiv, 1997 Solar neutrinos are discussed in the light of the new data and of recent progress in helioseismology. Most attention is given to the new status of Standard Solar Models due to seismically measured density and sound speed in the inner solar core. The elementary particle solutions to the Solar Neutrino Problem and their observational signatures are ...
arxiv
Neutrino dispersion relation changes due to radiative corrections as the origin of faster-than-light-in-vacuum propagation in a medium [PDF]
arXiv, 2011 Radiative corrections to the dispersion of neutrinos in nonstandard vacuum may give rise to "boosts" in their speed. This could explain recent experimental evidence by the OPERA collaboration, as well as the null result indicated by the supernova 1987A (SN 1987A) measurements of neutrino and photon arrival times.
arxiv
Super-resolution imaging for the detection of low-energy ion tracks in fine-grained nuclear emulsions. [PDF]
Sci Rep, 2023 Alexandrov A +4 more
europepmc +1 more source
in Neutrino 96, Proceedings of the 17th International Conference
on Neutrino Physics and Astrophysics, Helsinki, Finland, June 13-19, 1996,
eds. Kari Enqvist, Katri Huitu, and Jukka Maalampi (World Scientific,
Singapore, 1997), pp. 56-70, 1996 The neutrino fluxes calculated from 14 standard solar models published recently in refereed journals are inconsistent with the results of the 4 pioneering solar neutrino experiments if nothing happens to the neutrinos after they are created in the solar interior.
arxiv
Diffuse neutrino background from past core collapse supernovae. [PDF]
Proc Jpn Acad Ser B Phys Biol Sci, 2023 Ando S, Ekanger N, Horiuchi S, Koshio Y.
europepmc +1 more source
On velocities beyond the speed of light c [PDF]
arXiv, 1997 From a mathematical point of view velocities can be larger than c. It has been shown that Lorentz transformations are easily extended in Minkowski space to address velocities beyond the speed of light. Energy and momentum conservation fixes the relation between masses and velocities larger than c, leading to the possible observation of negative mass ...
arxiv
Search for High Energy Neutrino Emission from Gamma-Ray Bursts with the A ntarctic Muon and Neutrino Detector Array (AMANDA) [PDF]
arXiv, 2000 The photo-meson production of pions by shock-accelerated protons could generate a burst of ~10^14 eV neutrinos from gamma-ray bursts (GRBs) observable in the Antarctic Muon and Neutrino Detector Array (AMANDA) or its larger successors. Measurement of this flux can test the hypothesis that GRBs are the sources of the highest-energy cosmic rays, and GRB ...
arxiv
Results of Long-Baseline Neutrino Experiments Based on the Consideration of Frameworks [PDF]
arXiv, 2012 In this paper, we present an analysis of the outcomes of long-baseline neutrino experiments based on the consideration of frameworks. Our analysis suggests that the time difference between the time-of-flights corresponding to the speed of light (in vacuum) and that of the neutrino from a source to a detector is within the range of our predicted time ...
arxiv
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Comparison of muon and neutrino times from decays of mesons in the atmosphere [PDF]
arXiv, 2011 We propose a test to compare the speed of muons and muon neutrinos produced in the same bundles in the atmosphere. By comparing the arrival times of primary muons and muons induced by neutrinos, experiments such as Super-Kamiokande, IceCube and ANTARES could verify recent hints on the possibility that neutrinos have a velocity larger than the speed of ...
arxiv