Results 91 to 100 of about 241,115 (208)

The Era of Kilometer-Scale Neutrino Detectors

Advances in High Energy Physics, 2013
Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it was realized that kilometer-scale neutrino detectors were required.
Francis Halzen, Uli Katz
doaj   +1 more source

88th Annual Meeting of the Meteoritical Society 2026: Abstracts

Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley   +1 more source

Neutrino Constraints on Black Hole Formation in M31

The Open Journal of Astrophysics
We investigate neutrino signals associated with black hole formation resulting from the gravitational collapse of massive stars, motivated by the candidate failed supernova M31-2014-DS1 in the Andromeda Galaxy (M31).
Yudai Suwa, Ryuichiro Akaho, Yosuke Ashida, Akira Harada, Masayuki Harada, Yusuke Koshio, Masamitsu Mori, Fumi Nakanishi, Ken'ichiro Nakazato, Kohsuke Sumiyoshi, Roger A. Wendell, Masamichi Zaizen   +11 more
doaj   +1 more source

The role of neutrinos in explosive nucleosynthesis in core collapse supernova models with neutrino transport [PDF]

, 2007
The problem of core collapse supernova explosions is long standing and attempts to understand the mechanism have been ongoing. On one hand, a full understanding of the underlying mechanism is still pending.
Fröhlich, Carla
core   +1 more source

KM3NeT Online Multi-Messenger Results [PDF]

EPJ Web of Conferences
KM3NeT is a Cherenkov-light based neutrino telescope located in the Mediterranean Sea, comprising two detectors ARCA (Sicily, It) and ORCA (Var, Fr).
Carenini F., Cecchini V., Celli S., Dornic D., De Favereau J., Filippini F., Fusco L., Giorgio E., Le Guirriec E., Illuminati G., Lamoureux M., Magnani F., Marconi M., Mastrodicasa M., Palacios González J., Pastor Gómez E., Del Rosso I., Salesa Greus F., Sánchez Losa A., Le Stum S., Vannoye G., Veutro A.   +21 more
doaj   +1 more source

Superluminal velocity through near-maximal neutrino oscillations or by being off shell

, 2012
Recently it was suggested that the observation of superluminal neutrinos by the OPERA collaboration may be due to group velocity effects resulting from close-to-maximal oscillation between neutrino mass eigenstates, in analogy to known effects in optics.
Morris, Tim R.
core   +1 more source

An Introduction to Neutrino Astronomy

, 2021
The neutrino is a particle first theorized less than a century ago which has the unique properties of having mass but no electric charge. This allows the neutrino to move at extremely fast speeds through space, and through observation of these particles ...
Scott, Evelyn
core   +1 more source

Probing dark matter and phantom field effects on neutrino oscillations around black holes

European Physical Journal C: Particles and Fields
This study investigates how dark matter in the background of the phantom field (DMPF) near a black hole influences neutrino flavor oscillations using a two-flavor model.
Ikrom Ergashov, Bakhtiyor Narzilloev, Ibrar Hussain, Bobomurat Ahmedov   +3 more
doaj   +1 more source

Ultra High Energy Cosmic Rays, Z-Shower and Neutrino Astronomy by Horizontal-Upward Tau Air-Showers.

, 2003
Ultra High Cosmic Rays (UHECR) Astronomy may be correlated to a primary parental Neutrino Astronomy: indeed any far BL Lac Jet or GRB, sources of UHECR, located at cosmic edges, may send its signal, overcoming the severe GZK cut-off, by help of UHE ZeV ...
FARGION, Daniele
core  

On the energy and baseline optimization to study effects related to the δ-phase (CP-/T-violation) in neutrino oscillations at a neutrino factory [PDF]

, 2002
In this paper we discuss the detection of CP- and T-violation effects in the framework of a neutrino factory. We introduce three quantities, which are good discriminants for a non-vanishing complex phase (δ) in the 3 × 3 neutrino mixing matrix: Δδ, ΔCP ...
Navas-Concha, S, Rubbia, A, Campanelli, M, Bueno, A   +3 more
core