Neutrino clouds

被引：58
作者：
Stephenson, GJ [1 ]
Goldman, T
McKellar, BHJ
机构：
[1] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
[2] Univ Calif Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
[3] Univ Melbourne, Sch Phys, Parkville, Vic 3052, Australia
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 1998年 / 13卷 / 16期
关键词：
D O I：
10.1142/S0217751X98001414
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
We consider the possibility that neutrinos (but no other light fermions) are coupled very weakly to an extremely light scalar boson. We first analyze the simple problem of one generation of neutrino and show that, for ranges of parameters that are allowed by existing data, such a system can have serious consequences for the evolution of stars and could impact precision laboratory measurements. We discuss the extension to more generations and show that the general conclusion remains viable. Finally, we note that, should such a scalar field be present, experiments give information about effective masses, not the masses that arise in unified held theories.
引用
收藏
页码：2765 / 2790
页数：26
相关论文
共 30 条
  • [1] POSSIBLE GRAVITATIONAL MICROLENSING OF A STAR IN THE LARGE MAGELLANIC CLOUD
    ALCOCK, C
    AKERLOF, CW
    ALLSMAN, RA
    AXELROD, TS
    BENNETT, DP
    CHAN, S
    COOK, KH
    FREEMAN, KC
    GRIEST, K
    MARSHALL, SL
    PARK, HS
    PERLMUTTER, S
    PETERSON, BA
    PRATT, MR
    QUINN, PJ
    RODGERS, AW
    STUBBS, CW
    SUTHERLAND, W
    [J]. NATURE, 1993, 365 (6447) : 621 - 623
  • [2] PHYSICAL CONDITIONS IN THE INITIAL STAGES OF THE EXPANDING UNIVERSE
    ALPHER, RA
    FOLLIN, JW
    HERMAN, RC
    [J]. PHYSICAL REVIEW, 1953, 92 (06): : 1347 - 1361
  • [3] EVIDENCE FOR GRAVITATIONAL MICROLENSING BY DARK OBJECTS IN THE GALACTIC HALO
    AUBOURG, E
    BAREYRE, P
    BREHIN, S
    GROS, M
    LACHIEZEREY, M
    LAURENT, B
    LESQUOY, E
    MAGNEVILLE, C
    MILSZTAJN, A
    MOSCOSO, L
    QUEINNEC, F
    RICH, J
    SPIRO, M
    VIGROUX, L
    ZYLBERAJCH, S
    ANSARI, R
    CAVALIER, F
    MONIEZ, M
    BEAULIEU, JP
    FERLET, R
    GRISON, P
    VIDALMADJAR, A
    GUIBERT, J
    MOREAU, O
    TAJAHMADY, F
    MAURICE, E
    PREVOT, L
    GRY, C
    [J]. NATURE, 1993, 365 (6447) : 623 - 625
  • [4] MAJORON EMISSION BY NEUTRINOS
    BARGER, V
    KEUNG, WY
    PAKVASA, S
    [J]. PHYSICAL REVIEW D, 1982, 25 (03): : 907 - 910
  • [5] RESULTS OF THE TROITSK EXPERIMENT ON THE SEARCH FOR THE ELECTRON ANTINEUTRINO REST MASS IN TRITIUM BETA-DECAY
    BELESEV, AI
    BLEULE, AI
    GERASKIN, EV
    GOLUBEV, AA
    GOLUBEV, NA
    KAZACHENKO, OV
    KIEV, EP
    KUZNETSOV, YE
    LOBASHEV, VM
    OVCHINNIKOV, BM
    PARFENOV, VI
    SEKACHEV, IV
    SOLODUKHIN, AP
    TITOV, NA
    YARYKIN, IE
    ZAKHAROV, YI
    BALASHOV, SN
    SPIVAK, PE
    [J]. PHYSICS LETTERS B, 1995, 350 (02) : 263 - 272
  • [6] BERQVIST KE, 1972, NUCL PHYS B, V39, P317
  • [7] Binney J., 2008, GALACTIC DYNAMICS
  • [8] NON-NEWTONIAN GRAVITY AND NEW WEAK FORCES - AN INDEX OF MEASUREMENTS AND THEORY
    FISCHBACH, E
    GILLIES, GT
    KRAUSE, DE
    SCHWAN, JG
    TALMADGE, C
    [J]. METROLOGIA, 1992, 29 (03) : 213 - &
  • [9] DO EXPERIMENTS AND ASTROPHYSICAL CONSIDERATIONS SUGGEST AN INVERTED NEUTRINO MASS HIERARCHY
    FULLER, GM
    PRIMACK, JR
    QIAN, YZ
    [J]. PHYSICAL REVIEW D, 1995, 52 (02): : 1288 - 1291
  • [10] GOLDMAN T, 1981, PHYS REV D, V26, P2503
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