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| 001 | 387623 | ||
| 003 | ES-MaUEC | ||
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| 007 | cr nn 008mamaa | ||
| 008 | 230325s2020 sz | s |||| 0|eng d | ||
| 020 | _a9783031026126 | ||
| 024 | 7 |
_a10.1007/978-3-031-02612-6 _2doi |
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| 040 |
_aES-MaUEC _bspa _cES-MaUEC _dES-MaUEC |
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| 050 | 4 |
_aQC179 _b2020 EB |
|
| 100 | 1 |
_aBabak, Stanislav _eautor _4aut _4http://id.loc.gov/vocabulary/relators/aut _9687548 |
|
| 245 | 1 | 0 |
_aGravitational Waves from Coalescing Binaries _cby Stanislav Babak |
| 250 | _a1st edition 2020 | ||
| 264 | 1 |
_aCham _bSpringer International Publishing _c2020 |
|
| 300 | _a1 recurso en línea (VIII, 107 páginas) | ||
| 336 |
_atexto _btxt _2rdacontent |
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| 337 |
_aelectrónico _bc _2rdamedia |
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| 338 |
_arecurso electrónico _bcr _2rdacarrier |
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| 347 |
_aarchivo de texto _bPDF |
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| 490 | 0 |
_aSynthesis Lectures on Wave Phenomena in the Physical Sciences _x2690-2354 |
|
| 505 | 0 | _aIntroduction -- Gravitational Waves from Coalescing Binaries -- Gravitational Waves Data Analysis -- GW Sources and Observatories -- Bibliography -- Author's Biography. | |
| 520 | _aThis book is to help post-graduate students to get into gravitational wave astronomy. We assume the knowledge of General Relativity theory, though we will concentrate on the physics and often omit mathematically strict derivations. We provide references to already existing literature where possible, this helps us to see a broad picture, skipping the details. The uniqueness of this book is in that it covers three frequency bands and three major world-wide efforts to detect gravitational waves. The LIGO and Virgo scientific collaboration has detected first gravitational waves and the merger of black holes become now almost a routine. We do expect many discoveries yet to come, especially in the joined gravitational and electromagnetic observations. LISA, the space-based gravitational wave observatory, will be launched around 2034 and will be able to detect thousands of GW sources in the milli-Hz band. Pulsar timing array observations have accumulated 20-years' worth of data and we expected detection of GWs in the nano-Hz band within the next decade. We describe the gravitational wave sources and data analysis techniques in each frequency band. | ||
| 988 | _aSynthesis Collection of Technology_2020 | ||
| 650 | 7 |
_2embne _9687549 _aOndas gravitatorias |
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| 776 | 0 | 8 |
_iPrinted edition: _z9783031003561 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783031014840 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783031037405 |
| 856 | 4 | 0 |
_uhttps://go.openathens.net/redirector/universidadeuropea.es?url=https://doi.org/10.1007/978-3-031-02612-6 _zAcceso a este recurso digital (usuarios Universidad Europea de Madrid) |
| 942 |
_2lcc _cLE |
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| 998 |
_b03/2023 _dz _eIG _zSI |
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