Neutrino mass and detection of neutrino supernova bursts

Tsvi Piran

doi:10.1016/0370-2693(81)90880-7

Neutrino mass and detection of neutrino supernova bursts

Tsvi Piran^*

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

11 Scopus citations

Abstract

A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range m_{ν≳0.1 eV}.

Original language	English
Pages (from-to)	299-302
Number of pages	4
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	102
Issue number	4
DOIs	https://doi.org/10.1016/0370-2693(81)90880-7
State	Published - 18 Jun 1981
Externally published	Yes

Access to Document

10.1016/0370-2693(81)90880-7

Cite this

@article{e4f4a9633c8a433aa45e0b41b35c8033,

title = "Neutrino mass and detection of neutrino supernova bursts",

abstract = "A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range mν≳0.1 eV.",

author = "Tsvi Piran",

year = "1981",

month = jun,

day = "18",

doi = "10.1016/0370-2693(81)90880-7",

language = "אנגלית",

volume = "102",

pages = "299--302",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier B.V.",

number = "4",

}

TY - JOUR

T1 - Neutrino mass and detection of neutrino supernova bursts

AU - Piran, Tsvi

PY - 1981/6/18

Y1 - 1981/6/18

N2 - A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range mν≳0.1 eV.

AB - A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range mν≳0.1 eV.

UR - https://www.scopus.com/pages/publications/0038537903

U2 - 10.1016/0370-2693(81)90880-7

DO - 10.1016/0370-2693(81)90880-7

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:0038537903

SN - 0370-2693

VL - 102

SP - 299

EP - 302

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

IS - 4

ER -

Neutrino mass and detection of neutrino supernova bursts

Abstract

Access to Document

Other files and links

Fingerprint

Cite this