From first light to reionization: the end of the Dark Ages
This up-to-date and concise account of a critical period of the early universe directly links the latest theories and experiments. Targeted at cosmological problems rather than specific methods, it begins with an introduction reviewing the early universe and looks at why reionization is important.
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Weinheim
Wiley-VCH
2009
|
| Schlagworte: | |
| Online-Zugang: | Inhaltstext Inhaltsverzeichnis |
| Zusammenfassung: | This up-to-date and concise account of a critical period of the early universe directly links the latest theories and experiments. Targeted at cosmological problems rather than specific methods, it begins with an introduction reviewing the early universe and looks at why reionization is important. |
| Beschreibung: | XI, 218 S. graph. Darst. |
| ISBN: | 9783527407057 |
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Datensatz im Suchindex
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VII CONTENTS PREFACE V 1 INTRODUCTION 1 1.1 FIRST LIGHT AND REIONIZATION
1 1.2 THE COSMOLOGICAL FRAMEWORK 2 1.3 ORGANIZATION OF THIS BOOK 2 1.4
KEY OBSERVATIONS IN THIS FIELD 4 PART 1 THEORY 5 2 THE FIRST STARS 7 2.1
OVERVIEW 7 2.1.1 FIRST LIGHT 7 2.1.2 FORMING THE FIRST STARS 8 2.1.3 THE
LEGACY OF THE FIRST STARS 9 2.2 BEFORE THE FIRST STARS 9 2.2.1
RECOMBINATION AND RESIDUAL IONIZATION FRACTION 9 2.2.2 THE FORMATION OF
MOLECULAR HYDROGEN 13 2.2.3 COOLING FUNCTIONS 16 2.3 FORMING THE FIRST
STARS 18 2.3.1 PERTURBATIONS IN THE EARLY UNIVERSE 18 2.3.2 COLLAPSE OF
PERTURBATIONS IN THE EARLY UNIVERSE 21 2.3.3 COOLING AND THE JEANS
INSTABILITY 25 2.3.4 PROPERTIES OF THE FIRST STARS 31 2.3.5 REMNANTS AND
SIGNATURES OF A POPULATION III 34 2.4 PRIMORDIAL HI I REGIONS 35 2.5
WHAT IF DARK MATTER IS NOT COLD? 37 2.6 HINTS FOR FURTHER STUDY 38 3 THE
FIRST STAR CLUSTERS AND GALAXIES 39 3.1 OVERVIEW 39 3. BIBLIOGRAFISCHE
INFORMATIONEN HTTP://D-NB.INFO/991677196 DIGITALISIERT DURCH VIII
CONTENTS 3.2.3 LATE POPULATION III STAR FORMATION BY ATOMIC-HYDROGEN
COOLING IN MASSIVE HALOS 48 3.2.4 TERMINATION OF THE FIRST STARS PHASE
49 3.3 CONTAINING GAS IN THE HALOS OF POPULATION III STARS 49 3.3.1
IONIZATION HEATING AND GAS TEMPERATURE 49 3.3.2 THE ESCAPE OF GAS HEATED
BY IONIZATION 53 3.3.3 THE ESCAPE OF GAS FOLLOWING A SUPERNOVA EXPLOSION
56 3.3.4 POPULATION II.5 58 3.4 THE FIRST STAR CLUSTERS 59 3.4.1
CLUSTERS OF POPULATION III STARS AND OF METAL-POOR STARS 61 3.4.2 THE
ORIGIN OF GLOBULAR CLUSTERS 62 3.5 THE FIRST GALAXIES 63 3.6 THE FIRST
ACTIVE GALACTIC NUCLEI 64 3.6.1 POPULATION III BLACK HOLES 64 3.6.2
BLACK-HOLE MERGERS 65 3.6.3 THE HIGHEST-REDSHIFT QSOS 66 3.6.4 DIRECT
COLLAPSE TO BLACK HOLES 67 3.7 LOW-METALLICITY HII REGIONS 67 3.8
NUMERICAL TECHNIQUES AND THEIR LIMITATIONS 68 3.8.1 COLLISIONLESS
DYNAMICS 68 3.8.2 COLLISIONLESS DYNAMICS: PARTICLE-MESH CODES 70 3.8.3
COLLISIONLESS DYNAMICS: TREECODES 71 3.8.4 GAS DYNAMICS 71 3.8. CONTENTS
I IX 4.7 REHEATING OF THE INTERGALACTIC MEDIUM 97 4.8 KEEPING THE
INTERGALACTIC MEDIUM IONIZED 98 4.9 HINTS FOR FURTHER STUDY 100 PART 2
OBSERVATIONAL TECHNIQUES AND THEIR RESULTS 202 5 STUDYING THE EPOCH OF
REIONIZATION OF HYDROGEN 203 5.1 OVERVIEW 203 5.2 GUNN-PETERSON TROUGHS
IN REDSHIFT 6 QSOS 104 5.2.1 A SIMPLE GUNN-PETERSON TEST 204 5.2.2 THE
GUNN-PETERSON TROUGH 106 5.2.3 LYMAN SERIES LINES 208 5.2.4 METAL LINES
209 5.2.5 HII REGION SIZE TEST 209 5.2.6 DARK GAPS 220 5.2.7 AN
ASSESSMENT OF THE INDICATION FROM QSOS SPECTRA 220 5.3 LYMAN A SOURCES
AS DIAGNOSTICS OF REIONIZATION 222 5.3.1 EFFECT OF A FINITE LYMAN A LINE
WIDTH 2 11 5.3.2 INTRINSIC PROPERTIES OF LYMAN A EMITTERS 111 5.3.3
EFFECT OF A LOCAL IONIZED BUBBLE 2 14 5.3.4 A REALISTIC LYMAN A ESCAPE
MODEL 225 5.3.5 PERSPECTIVES ON STUDYING REIONIZATION WITH LYMAN A
SOURCES 117 5.3.6 FAINT LYMAN A HALOS 229 5.4 NEUTRAL-HYDROGEN SEARCHES
222 5.4.1 OTHER APPLICATIONS OF HIGH-Z 21-CM OBSERVATIONS 224 5.5
COMPTON OPTICAL DEPTH 226 5.6 LYMAN A SIGNATURE IN THE DIFFUSE NEAR-IR
BACKGROUND 227 5.7 HINTS FOR FURTHER STUDY 228 6 CONTENTS 6.8 DIRECT
DETECTION OF THE FIRST STARS 248 6.9 HINTS FOR FURTHER STUDY 249 7 DEEP
IMAGING AND SPECTROSCOPY SURVEYS 252 7.1 OVERVIEW 252 7.2 FIELD CHOICE
FOR A DEEP IMAGING SURVEY 252 7.3 OBSERVING TECHNIQUES FOR DEEP IMAGING
SURVEYS 254 7.3.1 GENERAL CONSIDERATIONS 154 7.3.2 DITHERING 254 7.3.3
SUPER BIAS AND SUPER DARK 255 7.3.4 FLAT FIELDING 256 7.3.5 IMAGE
COMBINATION 257 7.4 SELF-CALIBRATION 260 7.5 CATALOGS 162 7.5.1 LAYOUT
OF AN AUTOMATED PHOTOMETRY ALGORITHM 262 7.5.2 SEXTRACTOR PHOTOMETRY
TIPS 163 7.5.3 SIMULATIONS 164 7.6 COSMIC VARIANCE 266 7.7 THE
GRAVITATIONAL TELESCOPE 266 7.8 DEEP SPECTROSCOPY 269 7.8.1
SPECTROSCOPIC ANALYSIS TECHNIQUES 169 7.8.2 SLIT SPECTROSCOPY OF FAINT
TARGETS 270 7.8.3 SLITLESS SPECTROSCOPY 171 7.9 HINTS FOR FURTHER STUDY
272 8 THE REIONIZATION OF HELIUM 273 8.1 OVERVIEW 273 8.2 GUNN-PETERSON
TROUGHS IN QSOS 273 8.3 CONSTRAINTS FROM THE TEMPERATURE OF THE IGM 275
8.4 CHANGE IN METAL-LINE RATIOS 276 8.5 CHANGE IN HI LYMAN A FOREST 277
8.6 REIONIZING HYDROGEN FIRST AND HELIUM LATER 277 8.7 A LIMIT ON THE
ESCAPE FRACTION FROM GALAXIES AT Z ~ 3 278 9 FUTURE INSTRUMENTATION 282
9.1 OVERVIEW 282 9. CONTENTS XI 9.4.2 MULTIOBJECT SPECTROSCOPY 292 9.4.3
VERY HIGH RESOLUTION IMAGING 292 9.5 OBSERVING 21-CM RADIATION AT HIGH
REDSHIFT 192 9.5.1 MURCHISON WIDE-FIELD ARRAY 292 9.5.2 LOW-FREQUENCY
ARRAY 292 9.5.3 SQUARE-KILOMETER ARRAY 293 9.5.4 A RADIOTELESCOPE ON THE
FAR SIDE OF THE MOON 294 9.6 ATACAMA LARGE MILLIMITER ARRAY 194 9.7
LARGE FIELD OF VIEW IMAGING 194 9.7.1 LARGE SYNOPTIC SURVEY TELESCOPE
295 9.7.2 LARGE FIELD OF VIEW IMAGING FROM SPACE 295 9.8 PLANCK 195 A
OVERVIEW OF PHYSICAL CONCEPTS 197 A.I COSMOLOGICAL QUANTITIES 197 A.2
SAHA EQUATION 198 A. 3 POLYTROPIC STARS 200 A.4 JEANS INSTABILITY FOR A
TWO-FLUID SYSTEM 201 INDEX 223 |
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| spelling | Stiavelli, Massimo Verfasser aut From first light to reionization the end of the Dark Ages Massimo Stiavelli Weinheim Wiley-VCH 2009 XI, 218 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier This up-to-date and concise account of a critical period of the early universe directly links the latest theories and experiments. Targeted at cosmological problems rather than specific methods, it begins with an introduction reviewing the early universe and looks at why reionization is important. Beginning Cosmology Urknall (DE-588)4187224-1 gnd rswk-swf Urknall (DE-588)4187224-1 s DE-604 text/html http://deposit.dnb.de/cgi-bin/dokserv?id=3192007&prov=M&dok_var=1&dok_ext=htm Inhaltstext DNB Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=017368192&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
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| title | From first light to reionization the end of the Dark Ages |
| title_auth | From first light to reionization the end of the Dark Ages |
| title_exact_search | From first light to reionization the end of the Dark Ages |
| title_full | From first light to reionization the end of the Dark Ages Massimo Stiavelli |
| title_fullStr | From first light to reionization the end of the Dark Ages Massimo Stiavelli |
| title_full_unstemmed | From first light to reionization the end of the Dark Ages Massimo Stiavelli |
| title_short | From first light to reionization |
| title_sort | from first light to reionization the end of the dark ages |
| title_sub | the end of the Dark Ages |
| topic | Beginning Cosmology Urknall (DE-588)4187224-1 gnd |
| topic_facet | Beginning Cosmology Urknall |
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