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OCR for page 165
Index
A
Acceleration
cosmic-ray, 128
termination of, 130- 131
fractionation, 129, 130
galactic, 129
gravitation and, 15
shock, 128- 129
solar, 128
Actinide elements, 126, 127
Active masses, 23
Adiabatic perturbations, 95
Advanced X-Ray Astrophysics Facility
(AXAF), 101, 103- 104
Air showers, 120
Air-shower
detectors, 150
experiment, 140-141
observations, 130
Anisotropic cosmological models, 94
Anisotropy of space, 23
Antimatter, 148
Antinuclei, 138
Antiprotons, 116, 122, 136
Area Theorem, 64, 73
Astronomy
gamma-ray, 149-150, 151, 162
neutrino, 151 - 152, 163
165
Astronomy Survey Committee, 5, 157
Astrophysical properties of neutron stars
and black holes, 75, 76
· . .. ...
AStl Op ~yslcs ~ Vll-VllI
Atomic time versus solar-system time,
21 -22
AXAF (Advanced X-Ray Astrophysics
Facility), 101, 103-104
Axion forces, 78
Axions, 22, 97-98
B
Backaction-evasion technique, 44
Bar detectors, 43-44
observations with, 54
sensitivity and bandwidth, 52, 54
Bar-type gravity-wave detector, 44, 45
Baryon density, 90-92, 97
Baryons, 90
Beryllium, 122, 124
Big bang, initial singularity of, 65
Big-bang
models, 60, 87-89
nucleosynthesis, 90-92
Binary
pulsar, 14, 34-35, 39, 42-43
discovery of, 47
x-ray sources, 150
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1 66 INDEX
Black holes, 34-35, 36, 60
astrophysical properties of, 75, 76
colliding, 67, 68
as invisible mass, 97
quantum particle creation by, 64
rotating, 63
supermassive, 63
Black-hole
binary, 77
dynamics, four laws of, 64
jets, 26-27
Blackbody
curve, 93
radiation, primordial, 89
Cerenkov light, 131
Clocks
atomic versus gravitational, 22
gravitation effect on rate of, 18
hydrogen-maser, 18
Closure density of universe, 39, 100
COBE (Cosmic Background Explorer),
101, 103
Compact stars, systems of, 34-35
Computation, 58, 77
Computer technology, 110
Corkscrew jets, 27
Cosmic Background Explorer (COBE),
101, 103
Cosmic Censorship Hypothesis, 62, 64-
65, 72
Cosmic Ray Explorer, 6
Cosmic Ray Nuclei Experiment, 160
Cosmic rays, vii, 111 - 164
anomalous component, 132
connection with gamma and radio as-
tronomy7 137
correlation between anisotropy and en-
ergy, 135
energy dependence of escape from gal-
axy, 133-134
energy spectra of, 118, 119
galactic, 132- 133
extragalactic versus, 117
ground-based experiments with, 7, 149-
155, 161-164
high-energy composition and spectra,
146-147
high-energy nuclear and particle phys-
ics and, 137- 142
highlights, 121-142
hydrogen in, 129
interest in, 113-114
isotope ratios and, 125
large underground detectors for, 163-
164
major discoveries in, 121-123
opportunities, 143-156
origin of, 131
overview, 115- 120
primary, 133
principal recommendations in, 6-7
recommendations, 157- 164
secondaries from light nuclei, 135- 136
secondary, 133
solar, 131
solar modulation of, 149
solar-system material versus, 115-116
space program in, 6-7, 143-149, 157-161
theory of, 155- 156, 164
Cosmic strings, decaying, 48
Cosmic-ray
acceleration, 128
cascades, 120
detectors, nucleon decay experiments
as, 138-139
electrons, 135-136
isotopes, galactic, 144-145
lifetime, 136- 137
luminosity, 128
Cosmic-Ray Composition Explorer, 158,
159
Cosmological
constant, 74, 92
models
alternative, 107
anisotropic, 94
Cosmology, vii, 83-110
features of, 85-86
Grand Unification Theories and, 98-99
ground-based studies in, 6, 104-106,
109
highlights, 90-100
opportunities, 101-107
particle physics and, 106
principal recommendations in, 5-6
recommendations for, 108- 110
research, 6
space program in, 5, 101 - 104
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INDEX 1 67
standard model of, 87-89
theory of, 106- 107
CPT invariance, violation of, 78
D
Dark-matter problem, 86, 92, 96-98, 105-
106
Deceleration parameter, 92, 103
Deep Underwater Muon and Neutrino
Detector (DUMAND), l S 1, 163
Deuterium
abundance of, 92
observations of, 147
Deuterons, 90
Dipole effect, 94
Distance scale factor, 88
DUMAND (Deep Underwater Muon and
Neutrino Detector), 151, 163
E
Earth-Moon distance, 17, 27, 30-31
Eclipse observations, 19
Einstein equations, 65-66, 77
nonlinearities in, 66
Electromagnetic
field, 12
radiation, deflected, 19
signal retardation, 19-21
Electrons, cosmic-ray, 135- 136
Elementary particles, 88
Eotvos experiments, 1S, 17, 22
Equivalence principle, 15, 31
Escape length, cosmic-ray, 133
ETAP (Experimental Technical Assess-
ment Panel), 161
Euclidean functional integrals, 70
Expansion rate of universe, 103
Experimental Technical Assessment Pan-
el (ETAP), 161
Extragalactic radio sources, 93
F
Field equation, 13
Fly's Eye detector, 7, 140- 141, 150, 152,
162- 163
Fractionation, acceleration, 129, 130
Frame-dragging precession, 24-25
G
acceleration, 129
cosmic-ray isotopes, 144- 145
cosmic rays, 132- 133
formation, 89, 95
nuclei, 86
redshifts, 94-95
Galaxies, 86, 94
angular distributions of, 94
energy dependence of cosmic-ray es-
cape from, 133- 134
large-scale clustering of, 105
primeval, 102
Galileo mission, SS
Gamma Ray Observatory (GRO), 101
Gamma-ray
astronomy, 149- 150, 151, 162
bursters, 61
Gamma rays, 122
high-energy, 131
Gauge theories. 69
General relativity, 3
experimental tests of
highlights, 15-23
introduction, 11-14
opportunities, 24-35
Lagrangian for, 73-74
numerical techniques in' 67
Theory of, 60, 78-79
Geodetic precession, 25
GP-B (Gravity Probe B) (Relativity Gyro-
scope Experiment), 24-26, 31, 80
Grand unification mass scale, 78
Grand Unification Theories (GUTs), 78
cosmology and, 98-99
Gravitation, vii, 9-82; see curls`, Gravity
acceleration and, 15
binding energy, 15. 17, 68
clock versus atomic clock, 22
collapse, 62
constant, 92
changing, 21
rate of change of, 3
effect on rate of clocks. 18
effects, '~magnetic,'' 24-27
ground-based studies in, 4
laboratory testing of, 22-23
lenses, 100
progress in study of, 11
quadrupole moment of Sun, 33-34
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1 68 INDEX
recommendations in, 3-5, 80-82
redshift effect, 17- 18
solar-system tests of theories of, 16
space program for, 4
theory, 5
highlights, 61-71
introduction, 59-60
opportunities, 72-79
recommendations, 80-82
Gravitational waves, 4, 36, 60
detecting impulsive, 51
detecting periodic, 52
detecting stochastic, 53
emission of, 67
event rates and source calculations, 57
search for
highlights, 42-48
introduction, 36-41
opportunities, 49-58
sources of, 38-40
recent developments, 47-48
spacecraft tracking and, 55-56
theory of, 37
Gravitational-wave
background noise, 39
detectors, 40-41
Gravitino, 98
Gravitoelectric field, 12
Gravitomagnetic
effects, 24-27
field, 12
Graviton, nonlinear, 66
Gravity, 60; see also Gravitation
alternative theories of, 65
metric nature of, 3
quantization of, 106
quantum theory of, 59, 69-71, 73-75
Gravity Probe B (GP-B), 24-26, 31, 80
Gravity-wave detector, bar-type, 44, 45
GRO (Gamma Ray Observatory), 101
Ground-based studies
in cosmic rays, 7, 149-155, 161-164
in cosmology, 6
continued, 104- 106
recommendations for, 109
in gravitation, 4, 81
GUTs, see Grand Unification Theories
Gyroscopes, 24-26
H
H-space, 66
Hamiltonian of supergravity, 69
Hawking radiation, 59, 60, 64, 69
Heavy Nuclei Collector, 160
Helium, observations of, 147
HEPAP (High Energy Physics Advisory
Panel), 161
Higgs
fields, 99
particles, 106
High Energy Physics Advisory Panel
(HEPAP), 161
Hubble Space Telescope (HST), 101,
103, 104
Hubble's constant, 92, 100
Hubble's law, 94
Hughes-Drever experiments, 23
Hydrogen in cosmic rays, 129
Hydrogen-maser clock, 18
I
Impulsive gravitational waves, detecting,
51
Infinity, null, see Null infinity
Inflationary universe, 94, 99-100
Infrared Astronomy Satellite (IRAS),
101-102
Interferometric detectors, 44, 46
Invisible mass, 86, 92, 96-98, 105-106
IRAS (Infrared Astronomy Satellite),
101-102
Isotope
abundances, 91
ratios, cosmic rays and, 125
Isotopes, 144-145
galactic cosmic-ray, 144-145
solar-flare, 145
Isotropy, cosmological, 94
J
Jets, black-hole, 26-27
K
Kaluza-Klein theories, 71
Kerr solution to Einstein equations, 65
L
Lagrangian for general relativity, 73-74
Large Deployable Reflector (LDR), 101,
104
Large numbers hypothesis, 21
Laser interferometer detector, 40-41, 49-
52, 56-57, 81
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INDEX 1 69
Laser ranging, see Range measurements
LDEF (Long Duration Exposure Facili-
ty), 144, 146
LDR (Large Deployable Reflector), 101,
104
Leaky-box model, 136-137
Light deflection by Sun, 19
Light-element abundances, 91
Long Duration Exposure Facility
(LDEF), 144, 146
Long-Baseline Gravitational-Wave Facili-
ty, 4
Luminosity, cosmic-ray, 128
Lunar laser-ranging experiment, 17
M
MACRO (Monopole and Cosmic Ray Ob-
servatory), 152
"Magnetic" gravitational effects, 24-27
Magnetic monopoles, 99, 141-142, 153,
163
Mars Observer Mission, 29
Mass, missing, 86, 92, 96-98, 105-106
Mass-energy density, 87-88
Matter
missing, 86, 92, 96-98, 105-106
properties of, 85
Megaparsec (Mpc), 92
Mercury
perihelion advance of, 21
range measurements to, 28
Metric
hypothesis, 12- 13
nature of gravity, 3
Microwave background radiation, 85, 87,
89
absolute flux in, 93
anisotropy in, 95, 96
Millisecond pulsars, 46-47
Mis s ing matter, 86, 92, 96-98, 105- 106
Monopole and Cosmic Ray Observatory
(MACRO), 152
Monopoles, magnetic, 99, 141-142, 152-
153, 163
Moon, range measurements to, 17, 27,
30-31
Mossbauer effect, 18
Mpc (megaparsec), 92
Muons, 154, 164
N
Naive quantum limit, 44, 54
Naked singularity, 62
National Aeronautics and Space Admin-
istration (NASA), 3-4, 24, 55, 80,
101-104, 108, 157-161
National New Technology Telescope, 5,
109
National Science Foundation (NSF), 4,
49, 109-110, 161
Neutrino
astronomy, 151-152, 163
mass, 97
oscillation, 154
types, 106
Neutrinos, solar, 123, 126-127, 154-155,
164
Neutron stars, 34-35, 39, 61-62
astrophysical properties of, 75
mass limit for, 92
two, see Binary pulsar
Neutrons, 88
Nonlinear graviton, 66
NSF (National Science Foundation), 4
Nucleon, see Proton entries
Nucleosynthesis, 123-127
big-bang, 90-92
Nucleus-nucleus interactions, 139-140,
148-149
Null
experiments, 22
infinity, 66
angular momentum at, 73
complex spaces at, 79
o
Orbital motion, 43
p
Parameter is, PPN, 31-32
Parameterized-post-Newtonian (PPN)
formalism, 12-13
Particle Astrophysics Magnet Facility, 6
Particle physics, 71
cosmology and, 106
Particle-antiparticle annihilation, 88
Particles, elementary, 88
Passive masses, 23
Periastron precession, 35
Perihelion advance of Mercury, 21
Periodic gravitational waves, detecting,
52
Perturbation theory, 69-70
Perturbations, adiabatic, 95
Photino, 98
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1 70 INDEX
Photon barrier, 89, 93
Physics
cosmic-ray, see Cosmic rays
gravitation, see Gravitation
particle, see Particle physics
Planck era, 89, 99, 106
Planck mass scale, 78
POINTS (Precision Optical Interferome-
try in Space), 32-33, 81
Positive Energy Theorem, 68-69, 73-79
Positron-to-antiproton ratio, 147
Positrons, energy spectrum of, 136
PEN (parameterized-post-Newtonian) for-
malism, 12-13
Precession
frame-dragging, 24-25
geodetic, 25
periastron, 35
spin-orbit, 25
Precision Optical Interferometry in Space
(POINTS), 32-33, 81
Preferred-frame effects, 13
Primary cosmic rays, 133
Primeval galaxies, 102
Primordial blackbody radiation, 89
Proton decay, 99, 106
detectors, 153- 154, 163
as cosmic-ray detectors, 138-139 Rotating
experiments, 138-139
Proton-proton cross section, 123
Protons, 88
Pulsar
searches, 55
timing, 46-47
Pulsars, 39
binary, see Binary pulsar
millisecond, 46-47
radio, 46
x-ray, 55
Q
Quadrupole
anisotropy, 94
moment, gravitational, of Sun, 33-34
radiation, 43
Quantum
effects in early universe, 64-65
field theory in curved space-time, 69
particle creation by black holes, 64
theory of gravity, 59, 69-71, 73-75
Quantum-mechanical barrier penetration,
60
Quantum-nondemolition technique, 44
Quark-gluon
phase, 140
plasma, 148
Quarks, 88
Quasars, 63
R
Radar ranging, see Range measurements
Radio pulsar, 46
Radio sources, extragalactic, 93
Radio-interferometric techniques, 19
Range measurements
to Mercury, 4, 28
to Moon, 4, 17, 27, 30-31, 80
solar-system, 4, 27-28, 80
to Viking Landers on Mars, 28-29
Rapid reprocess, 124, 125-126
Redshift effect, gravitational, 17-18
Redshifts, galaxy, 94-95
Relativity, 59
general, see General relativity
solar-system tests of, 77-78
Relativity Gyroscope Experiment (GP-
B), 4, 24-26, 31, 80
black holes, 63
stars, 62
S
Scalar-tensor theory, 11
Scale factor, distance, 88
Secondary cosmic rays, 133
Shock acceleration, 128-129
Shuttle Infrared Telescope Facility
(SIRTF), 101, 102
Signal retardation, 19-21
Singularity
initial, of big bang, 65
naked, 62
theorems, 59
SIRTF (Shuttle Infrared Telescope Facil-
ity), 101, 102
Slow s-process, 124, 125-126
Solar
acceleration, 128
corona, 121
cosmic rays, 131
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INDEX
deflection of starlight, 32
flare isotopes, 145
modulation of cosmic rays, 149
neutrinos, 123, 126- 127, 154- 155, 164
quadrupole effect, 33-34
quadrupole moment, 29
system, 13
formation of, 124
measurements of dynamics of, 28
see also Sun entries
Solar-system
material, cosmic rays versus, 115- 116
range measurements, 27-28
tests, 4
of theories of gravitation, 16, 77-78
time versus atomic time, 21-22
Space
anisotropy of, 23
curvature, 12
program
in cosmic rays, 6-7, 143-149, 157-161
in cosmology, 5, 101-104, 108-109
in gravitation, 4, 80-81
Space Shuttle, 113
Space Station, 113, 143-144, 161
Space-curvature effects, 19
Space-time, 85
asymptotic properties of, 66-67, 72-73
curved, quantum field theory in, 69
foam, 74
origin of, 107
singularity, 62
Spacecraft tracking, gravitational waves
and, 55-56
Spectral density, strain, 44
Spin-orbit precession, 25
Spin-spin coupling, 25
SQUIDs (superconducting quantum inter-
ference devices), 54
Starlight, solar deflection of, 32
STARPROBE, 31, 81
Stochastic gravitational waves, detecting,
53
Strain sensitivity, 39, 43, 54
Strain spectral density, 44
Sun, see also Solar entries
light deflection by, 19
Sun-orbiting
laser interferometer, 41, 56-57, 81
Superconducting
coils, 153
171
quantum interference devices
(SQUIDs), 54
Superconducting Magnetic Spectrometer
Facility, 158- 159
Superconducting Super Collider, 5
Supergravity, 71
Hamiltonian of, 69
Supermassive black holes, 63
Supernova shock waves, 124
Supernovae, 38-39, 47, 103
Supersymmetric particle theories, 98
T
Termination of cosmic-ray acceleration,
130-131
Time-reversal invariance, violation of, 78
Twistor theory, 66
U
Ultraheavy elements, 145- 146
Ulysses spacecraft, 55, 149
Uniqueness Theorems, 63
Universe(s)
closure density of, 39, 100
early, quantum effects in, 64-65
expansion rate of, 103
history of, 87, 88
inflationary, 94, 99-100
large-scale properties of, 92-94
local, 86
simple, 60
structure in, 94-96
uniqueness of, 85
V
Very Long Baseline Array, 5, 109
Viking Landers, 20
range measurements to, 28-29
W
Weber bars, 40
Wormholes, 74
X
X-ray
pulsars, 55
sources, binary, 150
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Representative terms from entire chapter:
range measurements