A high-energy neutrino signature from supersymmetric relics

John S. Hagelin; K. W. Ng; Keith A. Olive

doi:10.1016/0370-2693(86)91205-0

A high-energy neutrino signature from supersymmetric relics

John S. Hagelin, K. W. Ng, Keith A. Olive

Physics and Astronomy (Twin Cities)

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

81 Scopus citations

Abstract

We compute the energy spectrum of high-energy (0.1-10 GeV) neutrinos produced by the annihilation of supersymmetric (SUSY) cold dark matter trapped in the sun. We compare this spectrum to the spectrum of atmospheric neutrinos and find that in the direction of the sun the solar flux of neutrinos can exceed the atmospheric background for neutrino energies E_ν {greater-than or approximate} 1 GeV, and are as much as a factor ∼ 30 above background for energies E_ν ∼ few GeV. We discuss these signatures for standard SUSY relics as well as for superstring relics.

Original language	English (US)
Pages (from-to)	375-380
Number of pages	6
Journal	Physics Letters B
Volume	180
Issue number	4
DOIs	https://doi.org/10.1016/0370-2693(86)91205-0
State	Published - Nov 20 1986

Bibliographical note

Funding Information:
We would like to thank D. Burke, S. Gasiorowicz, J. LoSecco, M. Srednicki and S. Rudaz for valuable discussions. The work of K.-W.N. and K.A.O. was supported in part by DOE grant DE-AC02-83ER-40105.

Publisher link

10.1016/0370-2693(86)91205-0

Find It

Find It at U of M Libraries

Cite this

@article{eef93cef354d4d6595ca4780a039d67f,

title = "A high-energy neutrino signature from supersymmetric relics",

abstract = "We compute the energy spectrum of high-energy (0.1-10 GeV) neutrinos produced by the annihilation of supersymmetric (SUSY) cold dark matter trapped in the sun. We compare this spectrum to the spectrum of atmospheric neutrinos and find that in the direction of the sun the solar flux of neutrinos can exceed the atmospheric background for neutrino energies Eν {greater-than or approximate} 1 GeV, and are as much as a factor ∼ 30 above background for energies Eν ∼ few GeV. We discuss these signatures for standard SUSY relics as well as for superstring relics.",

author = "Hagelin, {John S.} and Ng, {K. W.} and Olive, {Keith A.}",

note = "Funding Information: We would like to thank D. Burke, S. Gasiorowicz, J. LoSecco, M. Srednicki and S. Rudaz for valuable discussions. The work of K.-W.N. and K.A.O. was supported in part by DOE grant DE-AC02-83ER-40105.",

year = "1986",

month = nov,

day = "20",

doi = "10.1016/0370-2693(86)91205-0",

language = "English (US)",

volume = "180",

pages = "375--380",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier",

number = "4",

}

TY - JOUR

T1 - A high-energy neutrino signature from supersymmetric relics

AU - Hagelin, John S.

AU - Ng, K. W.

AU - Olive, Keith A.

N1 - Funding Information: We would like to thank D. Burke, S. Gasiorowicz, J. LoSecco, M. Srednicki and S. Rudaz for valuable discussions. The work of K.-W.N. and K.A.O. was supported in part by DOE grant DE-AC02-83ER-40105.

PY - 1986/11/20

Y1 - 1986/11/20

N2 - We compute the energy spectrum of high-energy (0.1-10 GeV) neutrinos produced by the annihilation of supersymmetric (SUSY) cold dark matter trapped in the sun. We compare this spectrum to the spectrum of atmospheric neutrinos and find that in the direction of the sun the solar flux of neutrinos can exceed the atmospheric background for neutrino energies Eν {greater-than or approximate} 1 GeV, and are as much as a factor ∼ 30 above background for energies Eν ∼ few GeV. We discuss these signatures for standard SUSY relics as well as for superstring relics.

AB - We compute the energy spectrum of high-energy (0.1-10 GeV) neutrinos produced by the annihilation of supersymmetric (SUSY) cold dark matter trapped in the sun. We compare this spectrum to the spectrum of atmospheric neutrinos and find that in the direction of the sun the solar flux of neutrinos can exceed the atmospheric background for neutrino energies Eν {greater-than or approximate} 1 GeV, and are as much as a factor ∼ 30 above background for energies Eν ∼ few GeV. We discuss these signatures for standard SUSY relics as well as for superstring relics.

UR - http://www.scopus.com/inward/record.url?scp=0001344329&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0001344329&partnerID=8YFLogxK

U2 - 10.1016/0370-2693(86)91205-0

DO - 10.1016/0370-2693(86)91205-0

M3 - Article

AN - SCOPUS:0001344329

SN - 0370-2693

VL - 180

SP - 375

EP - 380

JO - Physics Letters B

JF - Physics Letters B

IS - 4

ER -

A high-energy neutrino signature from supersymmetric relics

Abstract

Bibliographical note

Publisher link

Find It

Other files and links

Fingerprint

Cite this