Detecting the stochastic gravitational-wave background /
Saved in:
Author / Creator: | Colacino, Carlo Nicola, author. |
---|---|
Imprint: | San Rafael, CA : Morgan & Claypool Publishers, [2017] |
Description: | 1 volume (various pagings) : color illustrations ; 26 cm. |
Language: | English |
Series: | IOP concise physics, 2053-2571 IOP concise physics. |
Subject: | |
Format: | Print Book |
URL for this record: | http://pi.lib.uchicago.edu/1001/cat/bib/11563334 |
MARC
LEADER | 00000cam a2200000 i 4500 | ||
---|---|---|---|
001 | 11563334 | ||
005 | 20180412163230.8 | ||
008 | 180118s2017 caua b 000 0 eng d | ||
003 | ICU | ||
035 | |a (OCoLC)1019747880 | ||
040 | |a YDX |b eng |e rda |c YDX |d NhCcYBP | ||
020 | |a 1681740184 |q paperback | ||
020 | |a 9781681740188 |q paperback | ||
050 | 4 | |a QB817 |b .C654 2017 | |
082 | 0 | 4 | |a 523.8/2 |2 23 |
100 | 1 | |a Colacino, Carlo Nicola, |e author. |0 http://id.loc.gov/authorities/names/no2018084826 |1 http://viaf.org/viaf/187153061266219200620 | |
245 | 1 | 0 | |a Detecting the stochastic gravitational-wave background / |c Carlo Nicola Colacino. |
264 | 1 | |a San Rafael, CA : |b Morgan & Claypool Publishers, |c [2017] | |
300 | |a 1 volume (various pagings) : |b color illustrations ; |c 26 cm. | ||
336 | |a text |b txt |2 rdacontent |0 http://id.loc.gov/vocabulary/contentTypes/txt | ||
337 | |a unmediated |b n |2 rdamedia |0 http://id.loc.gov/vocabulary/mediaTypes/n | ||
338 | |a volume |b nc |2 rdacarrier |0 http://id.loc.gov/vocabulary/carriers/nc | ||
490 | 1 | |a IOP concise physics, |x 2053-2571 | |
500 | |a "Version: 20171201"--Title page verso. | ||
500 | |a "A Morgan & Claypool publication as part of IOP Concise Physics"--Title page verso. | ||
504 | |a Includes bibliographical references. | ||
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 Gravitational waves. |0 http://id.loc.gov/authorities/subjects/sh85056562 | |
650 | 7 | |a Gravitational waves. |2 fast |0 (OCoLC)fst00946882 | |
830 | 0 | |a IOP concise physics. |0 http://id.loc.gov/authorities/names/no2014089329 | |
903 | |a HeVa | ||
929 | |a cat | ||
999 | f | f | |i c000c1cc-5b2b-5af7-b3b4-d7c521554e28 |s aca91528-c36a-558a-b1e6-ffafefc84f41 |
928 | |t Library of Congress classification |a QB817 .C654 2017 |l JCL |c JCL-Sci |i 10910342 | ||
927 | |t Library of Congress classification |a QB817 .C654 2017 |l JCL |c JCL-Sci |e ALOFHARP |e crerar |b 114920158 |i 9956182 |