|
|
|
|
LEADER |
02572nam a2200397 i 4500 |
001 |
9781681740829 |
003 |
IOP |
005 |
20190313135847.0 |
006 |
m eo d |
007 |
cr cn |||m|||a |
008 |
180111s2017 caua ob 000 0 eng d |
999 |
|
|
|c 139879
|d 139879
|
020 |
|
|
|a 9781681740829
|q ebook
|
020 |
|
|
|a 9781681742106
|q mobi
|
020 |
|
|
|z 9781681740188
|q print
|
024 |
7 |
|
|a 10.1088/978-1-6817-4082-9
|2 doi
|
035 |
|
|
|a (CaBNVSL)thg00975460
|
035 |
|
|
|a (OCoLC)1019445691
|
040 |
|
|
|a CaBNVSL
|b gre
|e AACR2
|c GR-PaULI
|d GR-PaULI
|
072 |
|
7 |
|a SCI057000
|2 bisacsh
|
082 |
0 |
4 |
|a 523.82
|2 23
|
100 |
|
|
|a Colacino, Carlo Nicola
|e συγγραφέας.
|9 174593
|
245 |
1 |
0 |
|a Detecting the stochastic gravitational-wave background /
|c Carlo Nicola Colacino.
|
260 |
|
|
|a San Rafael [Καλιφόρνια] :
|b Morgan & Claypool Publishers,
|c c2017.
|
300 |
|
|
|a 1 ηλεκτρονική πηγή (ποικίλες σελιδαριθμήσεις) :
|b έγχρ. εικ.
|
490 |
1 |
|
|a IOP concise physics,
|x 2053-2571
|
504 |
|
|
|a Περιλαμβάνει βιβλιογραφικές παραπομπές.
|
505 |
0 |
|
|a 1. A brief history of gravitational radiation -- 1.1. Introduction -- 1.2. Sources of gravitational radiation -- 1.3. Gravitational waves from general relativity -- 1.4. Background reading
|
505 |
8 |
|
|a 2. General theoretical considerations about the cosmological SGWB -- 2.1. The SGWB and its detectability
|
505 |
8 |
|
|a 3. SGWB generation and source detection -- 3.1. Topological defects -- 3.2. Strings -- 3.3. Inflation -- 3.4. String cosmology
|
505 |
8 |
|
|a 4. Astrophysical sources -- 4.1. Conclusions.
|
520 |
3 |
|
|a The stochastic gravitational-wave background (SGWB) is by far the most difficult source of gravitational radiation detect. At the same time, it is the most interesting and intriguing one. This book describes the initial detection of the SGWB and describes the underlying mathematics behind one of the most amazing discoveries of the 21st century. On the experimental side it would mean that interferometric gravitational wave detectors work even better than expected. On the observational side, such a detection could give us information about the very early Universe, information that could not be obtained otherwise. Even negative results and improved upper bounds could put constraints on many cosmological and particle physics models.
|
650 |
|
0 |
|a Βαρυτικά κύματα
|9 174444
|
830 |
|
0 |
|a IOP concise physics.
|
856 |
4 |
0 |
|u http://iopscience.iop.org/book/978-1-6817-4082-9
|
942 |
|
|
|2 ddc
|c ERS
|