Neutrinos From Supernovae: Experimental Status

Cei, F.

doi:10.1142/9789812776808_0018

Cited by 2 publications

(6 citation statements)

References 12 publications

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“…A fairly updated general introduction and review of supernova neutrino physics is given in Refs. [41,42].…”

Section: Supernova Neutrinosmentioning

confidence: 99%

“…[42] and references therein). Many authors have studied future possibilities of supernova neutrino detection and its potential sensitivity to neutrino masses (see Refs.…”

Section: Futurementioning

confidence: 99%

“…Since most scientists are not so patient, there is an active research to study the feasibility of huge detectors that could observe a few tents of events produced by a supernova in the local group of galaxies (see Ref. [42] and references therein).…”

Section: Futurementioning

confidence: 99%

“…[26,37,38,39,40,41,42,43,44]). Actually, the intimate relationship of neutrinos and astrophysics goes even further back in time when Bethe and others realized that the inner workings of the Sun proceed via the thermonuclear reactions that burn hydrogen into helium and release neutrinos.…”

Section: Introductionmentioning

confidence: 99%

“…The role of neutrinos in Astrophysics and Cosmology has been under the scrutiny of physicists with ever increasing intensity over the last few decades (see Refs. [26,37,38,39,40,41,42,43,44]). Actually, the intimate relationship of neutrinos and astrophysics goes even further back in time when Bethe and others realized that the inner workings of the Sun proceed via the thermonuclear reactions that burn hydrogen into helium and release neutrinos.…”

Section: Introductionmentioning

confidence: 99%

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Absolute values of neutrino masses: status and prospects

et al. 2003

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Compelling evidences in favor of neutrino masses and mixing obtained in the last years in Super-Kamiokande, SNO, KamLAND and other neutrino experiments made the physics of massive and mixed neutrinos a frontier field of research in particle physics and astrophysics. There are many open problems in this new field. In this review we consider the problem of the absolute values of neutrino masses, which apparently is the most difficult one from the experimental point of view. We discuss the present limits and the future prospects of β-decay neutrino mass measurements and neutrinoless double-β decay. We consider the important problem of the calculation of nuclear matrix elements of neutrinoless double-β decay and discuss the possibility to check the results of different model calculations of the nuclear matrix elements through their comparison with the experimental data. We discuss the upper bound of the total mass of neutrinos that was obtained recently from the data of the 2dF Galaxy Redshift Survey and other cosmological data and we discuss future prospects of the cosmological measurements of the total mass of neutrinos. We discuss also the possibility to obtain information on neutrino masses from the observation of the ultra highenergy cosmic rays (beyond the GZK cutoff). Finally, we review the main aspects of the physics of core-collapse supernovae, the limits on the absolute values of neutrino masses from the observation of SN1987A neutrinos and the future prospects of supernova neutrino detection.1

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“…A fairly updated general introduction and review of supernova neutrino physics is given in Refs. [41,42].…”

Section: Supernova Neutrinosmentioning

confidence: 99%

“…[42] and references therein). Many authors have studied future possibilities of supernova neutrino detection and its potential sensitivity to neutrino masses (see Refs.…”

Section: Futurementioning

confidence: 99%

Section: Futurementioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

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Absolute values of neutrino masses: status and prospects

et al. 2003

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Detection of a close supernova gravitational wave burst in a network of interferometers, neutrino and optical detectors

Arnaud

Barsuglia

Bizouard

et al. 2004

Astroparticle Physics

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Trying to detect the gravitational wave (GW) signal emitted by a type II supernova is a main challenge for the GW community. Indeed, the corresponding waveform is not accurately modeled as the supernova physics is very complex; in addition, all the existing numerical simulations agree on the weakness of the GW emission, thus restraining the number of sources potentially detectable. Consequently, triggering the GW signal with a confidence level high enough to conclude directly to a detection is very difficult, even with the use of a network of interferometric detectors. On the other hand, one can hope to take benefit from the neutrino and optical emissions associated to the supernova explosion, in order to discover and study GW radiation in an event already detected independently. This article aims at presenting some realistic scenarios for the search of the supernova GW bursts, based on the present knowledge of the emitted signals and on the results of network data analysis simulations. Both the direct search and the confirmation of the supernova event are considered. In addition, some physical studies following the discovery of a supernova GW emission are also mentioned: from the absolute neutrino mass to the supernova physics or the black hole signature, the potential spectrum of discoveries is wide.

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Neutrinos From Supernovae: Experimental Status

Cited by 2 publications

References 12 publications

Absolute values of neutrino masses: status and prospects

Absolute values of neutrino masses: status and prospects

Detection of a close supernova gravitational wave burst in a network of interferometers, neutrino and optical detectors

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