Overduin J.M., Wesson P.S. — Dark sky, dark matter :: Электронная библиотека попечительского совета мехмата МГУ

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Overduin J.M., Wesson P.S. — Dark sky, dark matter

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Название: Dark sky, dark matter

Авторы: Overduin J.M., Wesson P.S.

Аннотация:

The approach of the authors is to compare the best observational data from large telescopes with the best cosmological theory based on general relativity and particle physics. Gives a more accurate picture of the universe and the exotic material believed to constitute dark matter.

Язык:

Рубрика: Физика/Гравитационное взаимодействие/Космология/

Статус предметного указателя: Готов указатель с номерами страниц

ed2k: ed2k stats

Год издания: 2003

Количество страниц: 216

Добавлена в каталог: 29.09.2005

Операции: Положить на полку | Скопировать ссылку для форума | Скопировать ID

Предметный указатель

Massive compact halo objects (MACHOs)      72 74
Matter density $({\rho}_{m})$       23 99
Matter density parameter $({\Omega}_{m,0})$       25 67 85 130
Matter density parameter $({\Omega}_{m,0}),$ evolution of $({\Omega}_{m})$       85
Matter radiation equality epoch of $({t}_{eq})$       97 100
Matter-antimatter annihilation      95
Maxima      83
Metric tensor $({g}_{\mu\nu})$       17
MeV bump, demise of      164
Microlensing      72
Milky Way, dynamical mass      74 118 130 155
Milky Way, luminosity (B band)      74
Milne model      see “Cosmological models”
Minimal supersymmetric model (MSSM)      147
Naked singularities      188
Neutralinos      147
Neutralinos, annihilation cross section      150 151
Neutralinos, bolometric intensity due to      152 155
Neutralinos, decay      see “WIMP decay”
Neutralinos, decay lifetime $({\tau}_{\chi})$       154 156 166
Neutralinos, in halos      see “WIMP halos”
Neutralinos, rest mass $({\tau}_{\tilda{\chi}})$       147
Neutralinos, spectral intensity due to      153 155 159
Neutrino decay      127 150
Neutrino decay, Feynman diagrams      129
Neutrino decay, lifetime $({\tau}_{v})$       127
Neutrino decay, spectral intensity due to      141
Neutrino halos      128
Neutrino halos, bolometric intensity due to      133
Neutrino halos, efficiency factor $(\epsilon)$       129 132 206
Neutrino halos, ellipsoidal density profile      131 206
Neutrino halos, luminosity $({L}_{h})$       129 133
Neutrino halos, mass $({M}_{h})$       130
Neutrino halos, spectral intensity due to      140
Neutrino oscillation      78
Neutrinoless double beta decay      78
Neutrinos      13 67 192
Neutrinos, blackbody temperature $({T}_{v})$       103
Neutrinos, bound      see “Neutrino halos”
Neutrinos, density parameter $({\Omega}_{v})$       61 11 78 103 130
Neutrinos, free streaming      see “Free-streaming neutrinos”
Neutrinos, in clusters of galaxies      128
Neutrinos, number density $({n}_{v})$       16
Neutrinos, rest mass $({m}_{v})$       11 127
Neutrinos, sterile      193
Neutron stars      72
Non-minimal coupling      92
Nucleosynthesis, primordial      71 94 98 161
Nucleosynthesis, stellar      5
OAO      2 49 121 142
OGLE microlensing survey      69
Olbers paradox      1
Olbers paradox, and absorption      3 64
Olbers paradox, and astronomy textbooks      4
Olbers paradox, and expansion      4 8 35 64 192
Olbers paradox, and finite age      4 7 35 64 192
Olbers paradox, and galaxy distribution      3
Olbers paradox, and spatial curvature      4
Olbers paradox, and the laws of physics      4
Olbers paradox, bolometric resolution of      35
Olbers paradox, in de Sitter model      31
Olbers paradox, spectral resolution of      63
Optical band      10 120
Optical depth      135 207
Optical depth, in dust      136
Optical depth, in neutral hydrogen      136
Pair production      156 158 181
PBHs      see “Primordial black holes”
Peccei — Quinn (PQ) symmetry      113
Phase transition      97 173
Photinos      147 150
Pioneer      10 46 49 121
Planck      84
Planck function      51
Planck s law      8
Primordial black holes (PBHs)      170 192
Primordial black holes (PBHs), and $\gamma$ -ray bursts      173
Primordial black holes (PBHs), and $\gamma$ -ray emission from halo      173
Primordial black holes (PBHs), and MACHO events      173
Primordial black holes (PBHs), and quasar variability      173
Primordial black holes (PBHs), bolometric intensity due to      180—182
Primordial black holes (PBHs), comovmg number density      175
Primordial black holes (PBHs), cut-off mass      180
Primordial black holes (PBHs), density $({\rho}_{pbh})$       176
Primordial black holes (PBHs), density parameter ${\Omega}_{pbh}$       176 181 185
Primordial black holes (PBHs), direct detection      185
Primordial black holes (PBHs), equation of state parameter $\beta$       175
Primordial black holes (PBHs), formation of during phase transition      173
Primordial black holes (PBHs), formation of via collapse of small density fluctuations      172
Primordial black holes (PBHs), formation of via cosmic string loops      173
Primordial black holes (PBHs), formation of via critical collapse      173 186
Primordial black holes (PBHs), formation of via inflationary mechanisms      172 186
Primordial black holes (PBHs), initial mass distribution      172
Primordial black holes (PBHs), lifetime $({t}_{pbh})$       174
Primordial black holes (PBHs), local evaporation rate      185
Primordial black holes (PBHs), luminosity      179
Primordial black holes (PBHs), normalization (N)      175 185
Primordial black holes (PBHs), photosphere      186
Primordial black holes (PBHs), spectral intensity due to      183 184
Primordial black holes (PBHs), stable relics      186
Primordial black holes (PBHs), typical mass ${M}_{*}$       175
Prognoz      142
Pure luminosity evolution (PLE)      52
Quantum chromodynamics (QCD)      79 113
Quark and gluonjets      185
Quark hadron transition      173 176
Quasars      3
Quasars, lensing frequency      81

Quasars, spectra      see “Lyman a absorbers”
Quasars, turnoff      136
Quasars, variability      72 173
Quintessence      23 67 92
R parity      147 154 161 167
Radiation density ${\rho}_{r}$       23 99
Radiation density parameter $({\Omega}_{r\;0})$       25 67 104
Radio galaxy lobes      75
Red clump stars      69
Red dwarfs      72
Redshift (z)      6 20
Ricci tensor in 4, dimensions ${\cal R}_{\mu\nu}$       17
Ricci tensor in 5, dimensions ${\cal R}_{AB}$       187
Robertson Walker metric      17
S electrons      147
SAGE      78
SAS      2 153 156 160 164 184
Scalar field      23 90 91
Scalar tensor theories      92
Schwarzschild metric      187
SCP      81
sed      see “Spectral energy distribution”
Sloan Digital Sky Survey (SDSS)      21 61
Sneutrinos      147
Soliton metric      187
Solitons      171 192
Solitons, density profile      188 189
Solitons, gravitational mass      188
Solitons, local energy density $({\rho}_{s})$       189
Solrad-11      142
Spectral energy distribution      42
Spectral energy distribution, blackbody      52 106 177
Spectral energy distribution, delta-function      44
Spectral energy distribution, Gaussian      50 121 129 150
Spectral energy distribution, inverse Compton scattering      158
Spectral energy distribution, inverse Compton scattering, with cascades      158
Spectral energy distribution, normalization      42
Spectral energy distribution, primordial black hole      177
Static analogue, bolometric intensity      28
Static analogue, spectral intensity      43
Steady-state theory      3
Stefan's law      52 103 107
String theory      194
Strong-CP problem      113 167
Subaru Deep Field      61
Sunyaev Zeldovich (SZ) effect      68
Super Kamiokande      78
Supernovae Type la (SNIa)      81 94 114 164
Supersymmetry      127 146 174
SUSY      see “Supersymmetry”
Total density parameter $({\Omega}_{\rot\;0})$       25 26
Two Degree Field (2dF)      21
Ultraviolet (UV) band      11 150
Ultraviolet (UV) band, extreme ultraviolet (EUV)      128
Ultraviolet (UV) band, far ultraviolet (FUV)      128
Ultraviolet (UV) band, near ultraviolet (NUV)      48 128
Unified field theory      16
Vacuum decay      13 90
Vacuum decay, and cosmic microwave background      95
Vacuum decay, bolometric intensity of      106
Vacuum decay, branching ratio $\beta$       103 104
Vacuum decay, comoving luminosity density of $({\cal L}_{V,0})$       105
Vacuum decay, coupling parameter (x)      97
Vacuum decay, into baryons      95
Vacuum decay, into radiation      95 97
Vacuum decay, luminosity $({L}_{V})$       104
Vacuum decay, luminosity $({L}_{V})$ , relativistic      102
Vacuum decay, luminosity $({L}_{V})$ , thermodynamical      102
Vacuum decay, phenomenological model      95
Vacuum decay, source regions      101
Vacuum decay, spectral intensity of      108
Vacuum density $({\rho}_{V})$       23 99
Vacuum density $({\rho}_{V})$ in terms of $\Lambda({\rho}_{V})$       24 79 96
Vacuum density parameter $({\Omega}_{\Lambda\;0})$       25 78 82 83 85
Vacuum density parameter $({\Omega}_{\Lambda\;0})$ , evolution of $({\Omega}_{\Lambda})$       85
Vacuum energy      67 78 192
Variable cosmological term      80 90
Velocity dispersion      121 129 150
Very massive objects (VMOs)      193
VIRGO consortium      81
Voyager      2 142
Warm dark matter (WDM)      193
Weakly-interacting massive particles (WIMPs)      13 76 146 192
Weakly-interacting massive particles (WIMPs), cosmological enhancement factor $({f}_{c})$       152
Weakly-interacting massive particles (WIMPs), decay      see “WIMP decay”
Weakly-interacting massive particles (WIMPs), direct detection of      148
Weakly-interacting massive particles (WIMPs), in halos      see “WIMP halos”
Weakly-interacting massive particles (WIMPs), indirect detection of      148
Weakly-interacting massive particles (WIMPs), pair annihilation of      146
Weakly-interacting massive particles (WIMPs), pair annihilation of, Feynman diagrams      149
Whipple collaboration      185
White dwarfs      72
Wien's Law      44
WIMP decay, branching ratio      155 158 162
WIMP decay, Feynman diagrams      154 157
WIMP decay, one-loop      147 154 165
WIMP decay, tree-level      147 157 161
WIMP halos      150
WIMP halos, cosmological density of      151
WIMP halos, density profile      see “Isothermal density profile”
WIMP halos, luminosity of      150 152 154 155 158 159 162
WIMPS      see “Weakly-interacting massive particles”
WIMPzillas      193
X ray band      11 147 160 193
X ray band, hard      164
X ray band, soft      164
Zero-point field (ZPF)      67
Zinos      147 151
Zodiacal light      46

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