Astrophysical Limits on Neutrino MASS for ${\boldsymbol m}_{{{\boldsymbol \nu}}}$ $>$ 1 GeV INSPIRE search

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
$\text{none 60 - 115}$ 1
FARGION
1995
ASTR Dirac
$\text{none 9.2 - 2000}$ 2
GARCIA
1995
COSM Nucleosynthesis
$\text{none 26 - 4700}$ 2
BECK
1994
COSM Dirac
$\text{none 6 - hundreds}$ 3, 4
MORI
1992B
 KAM2 Dirac neutrino
$\text{none 24 - hundreds}$ 3, 4
MORI
1992B
 KAM2 Majorana neutrino
$\text{none 10 - 2400}$ 90 5
REUSSER
1991
CNTR HPGe search
$\text{none 3 - 100}$ 90
SATO
1991
KAM2 Kamiokande II
6
ENQVIST
1989
COSM
$\text{none 12-1400}$ 2
CALDWELL
1988
COSM Dirac ${{\mathit \nu}}$
$\text{none 4-16}$ 90 3, 2
OLIVE
1988
COSM Dirac ${{\mathit \nu}}$
$\text{none 4-35}$ 90
OLIVE
1988
COSM Majorana ${{\mathit \nu}}$
$\text{>4.2 to 4.7}$
SREDNICKI
1988
COSM Dirac ${{\mathit \nu}}$
$\text{>5.3 to 7.4}$
SREDNICKI
1988
COSM Majorana ${{\mathit \nu}}$
$\text{none 20-1000}$ 95 2
AHLEN
1987
COSM Dirac ${{\mathit \nu}}$
$>4.1$
GRIEST
1987
COSM Dirac ${{\mathit \nu}}$
1  FARGION 1995 bound is sensitive to assumed ${{\mathit \nu}}$ concentration in the Galaxy. See also KONOPLICH 1994 .
2  These results assume that neutrinos make up dark matter in the galactic halo.
3  Limits based on annihilations in the sun and are due to an absence of high energy neutrinos detected in underground experiments.
4  MORI 1992B results assume that neutrinos make up dark matter in the galactic halo. Limits based on annihilations in earth are also given.
5  REUSSER 1991 uses existing ${{\mathit \beta}}{{\mathit \beta}}$ detector (see FISHER 1989 ) to search for CDM Dirac neutrinos.
6  ENQVIST 1989 argue that there is no cosmological upper bound on heavy neutrinos.
  References:
FARGION 1995
PR D52 1828 Bounds on very Heavy Relic Neutrinos by their Annihilation in Galactic Halo
GARCIA 1995
PR D51 1458 Results of a Dark Matter Search with a Germanium Detector in the Canfranc Tunnel
BECK 1994
PL B336 141 Searching for Dark Matter with the Enriched ${}^{}\mathrm {Ge}$ Detectors of the Heidelberg-Moscow Double $\beta $ Decay Experiment
MORI 1992B
PL B289 463 A Limit on Massive Neutrino Dark Matter from Kamiokande
REUSSER 1991
PL B255 143 Limits on Cold Dark Matter from the Gotthard ${}^{}\mathrm {Ge}$ Experiment
SATO 1991
PR D44 2220 Mass Limits for Dark Matter Particles Derived from High Energy Neutrinos from the Sun
ENQVIST 1989
NP B317 647 Cosmic Abundances of Very Heavy Neutrinos
CALDWELL 1988
PRL 61 510 Laboratory Limits on Galactic Cold Dark Matter
OLIVE 1988
PL B205 553 Solar Neutrino Searches and Cold Dark Matter
SREDNICKI 1988
NP B310 693 Calculations of Relic Densities in the Early Universe
AHLEN 1987
PL B195 603 Limits on Cold Dark Matter Candidates from an Ultralow Background Germanium Spectrometer
GRIEST 1987
NP B283 681 Cosmic Asymmetry, Neutrinos, and the Sun
KONOPLICH 1994
PAN 57 425 Cosmological Constraints on Very Heavy Stable Neutrinos