Solar neutrinos: probing the quasi-isothermal solar core produced by supersymmetric dark matter particles - Wikidata - wikimedia - TriplyDB

Solar neutrinos: probing the quasi-isothermal solar core produced by supersymmetric dark matter particles

Solar neutrinos: probing the quasi-isothermal solar core produced by supersymmetric dark matter particles

http://www.wikidata.org/entity/Q57220964

about

Indirect detection of light neutralino dark matter in the next-to-minimal supersymmetric standard model Light WIMPs in the Sun: Constraints from helioseismology Neutrino Spectroscopy Can Probe the Dark Matter Content in the Sun

P2860

Q56068304-B87C699D-7106-4D4F-83D9-59FE24B19A5E Q56934002-2D4082B1-585E-4829-8CA1-3C988F0C6631 Q56934007-6EA092FD-FD72-40D5-8CE0-E085A98B8F2D

P2860

Solar neutrinos: probing the quasi-isothermal solar core produced by supersymmetric dark matter particles

http://www.wikidata.org/entity/Q57220964

description

article publié dans la revue scientifique Physical Review Letters

@fr

im April 2002 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Physical Review Letters

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована у квітні 2002

@uk

name

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@en

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@nl

type

label

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@en

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@nl

prefLabel

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@en

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@nl

P1433

Q57220964-76686A9C-676F-46AB-9B06-AA3A9B834B39

P1476

Q57220964-407D1B01-7FBB-49C3-A4D0-13A71E6D9017

P2093

Q57220964-2D759692-B503-4922-930E-126BF12577F0

P2860

Q57220964-079DA128-C8C5-4BCC-BBDB-7D07559727E8

Q57220964-1E0D4BE3-A5D0-4786-B053-8C57090A6AFF

Q57220964-24D29B8C-5CDB-4217-9257-B618852E074F

Q57220964-4A54089E-5F3C-4E69-9A4D-445A8BB2627B

Q57220964-95A4A767-EF0C-46C0-8E07-3277C80E11F0

Q57220964-F6FE088D-C109-4E15-BEE3-8CC22C347D14

P304

Q57220964-FF6199E0-800B-499D-835F-7EEA75B46BAC

P31

Q57220964-C08750D8-614D-4285-8776-610D945FCA2F

P356

Q57220964-DBF3359A-44BC-4714-B12C-AE7375BC3220

P407

Q57220964-E3C005CF-B76D-4361-A770-B61D96964D49

P433

Q57220964-A6CF74A0-852A-4FCD-8891-F16D9618A497

P478

Q57220964-FC847943-BB0C-4F02-8B57-A7705A831585

P50

Q57220964-C9712B40-BAB5-4477-A740-B5B524C6C310

P577

Q57220964-F0D1A22D-C1F4-4EA4-A752-2C608D908FAC

P698

Q57220964-FFD62A99-B20E-4528-87DF-76B0A482C762

P818

Q57220964-5B4451C4-AED4-45CC-910B-81BD1BEBD44D

P921

Q57220964-7865FC46-B805-4EB8-BBB5-E4466183D090

Q57220964-D4E642A4-EF8A-4292-9ED7-CCCDC1677A8F

P356

PHYSREVLETT.88.151303

P1433

Physical Review Letters

P1476

Solar neutrinos: probing the q ...... ymmetric dark matter particles

@en

P2093

Ilídio P Lopes

http://www.w3.org/2001/XMLSchema#string

P2860

Measurement of the Rate of ν e + d → p + p + e − Interactions Produced by B 8 Solar Neutrinos at the Sudbury Neutrino Observatory

Supersymmetric dark matter

High-energy physics. Neutrinos reveal split personalities.

The Seismic Structure of the Sun

Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties

SolarB8and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data

P304

151303

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

P356

10.1103/PHYSREVLETT.88.151303

http://www.w3.org/2001/XMLSchema#string

P407

P433

15

http://www.w3.org/2001/XMLSchema#string

P478

88

http://www.w3.org/2001/XMLSchema#string

P50

P577

2002-04-15T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P698

11955186

http://www.w3.org/2001/XMLSchema#string

P818

astro-ph/0112390

http://www.w3.org/2001/XMLSchema#string

P921