The Gravitational Universe
The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as ou...
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| creator | Audley, H Auger, G Babak, S Baker, J Barausse, E Barke, S Benacquista, M Bender, P L Berti, E Binétruy, P Bogenstahl, J Bonvin, C Brossard, J Caprini, C Cavalleri, A Colpi, M Conklin, J Cornish, N Danzmann, K DeBra, D L Di Fiore M Diaz Aguilo Diepholz, I Dolesi, R Dotti, M G Fernández Barranco Ferraioli, L Finetti, N Fitzsimons, E Galeazzi, F Garcia, A Giardini, D Gibert, F Grimani, C Haiman, Z Halloin, H Heinzel, G Hewitson, M Hogan, C Hornstrup, A Hoyle, C D Hughes, S Kalogera, V Karnesis, N Killow, C Kochkina, E Korsakova, N Larson, S Livas, J Lloro, I Maghami, P Marsh, T Mateos, I Mayer, L McKenzie, K Merkowitz, S Miller, C Mitryk, S Moerschell, J Mohanty, S Monsky, A Mueller, G Müller, V Nelemans, G Nicolodi, D Nissanke, S Nofrarias, M Ohme, F Otto, M Perreur-Lloyd, M Plagnol, E Prat, P Reiche, J Richstone, D Robertson, D Rubbo, L Schlamminger, S Schütze, D Shah, S Sheard, B Spector, A Stanga, R Stebbins, R Stede, G Steier, F Sumner, T Sun, K -X Thorpe, I Tröbs, M Tinto, M H -B Tu Vetrugno, D Wang, Y Wanner, G Ward, H Ware, B Wass, P Weber, W J Y Yu Zweifel, P |
| description | The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it possible to trace the history of black holes across all stages of galaxy evolution, and at the same time constrain any deviation from the Kerr metric of General Relativity. eLISA will be the first ever mission to study the entire Universe with gravitational waves. eLISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the early processes at TeV energies, has guaranteed sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales around singularities and black holes, all the way to cosmological dimensions. |
| format | Article |
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We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it possible to trace the history of black holes across all stages of galaxy evolution, and at the same time constrain any deviation from the Kerr metric of General Relativity. eLISA will be the first ever mission to study the entire Universe with gravitational waves. eLISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the early processes at TeV energies, has guaranteed sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales around singularities and black holes, all the way to cosmological dimensions.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Big bang cosmology ; Black holes ; Cosmology ; Electromagnetic radiation ; Galactic evolution ; Galaxies ; Gravitation ; Gravitational waves ; Ionization ; Milky Way Galaxy ; Relativity ; Singularities ; Stellar evolution ; Universe</subject><ispartof>arXiv.org, 2013-05</ispartof><rights>2013. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780</link.rule.ids></links><search><creatorcontrib>Audley, H</creatorcontrib><creatorcontrib>Auger, G</creatorcontrib><creatorcontrib>Babak, S</creatorcontrib><creatorcontrib>Baker, J</creatorcontrib><creatorcontrib>Barausse, E</creatorcontrib><creatorcontrib>Barke, S</creatorcontrib><creatorcontrib>Benacquista, M</creatorcontrib><creatorcontrib>Bender, P L</creatorcontrib><creatorcontrib>Berti, E</creatorcontrib><creatorcontrib>Binétruy, P</creatorcontrib><creatorcontrib>Bogenstahl, J</creatorcontrib><creatorcontrib>Bonvin, C</creatorcontrib><creatorcontrib>Brossard, J</creatorcontrib><creatorcontrib>Caprini, C</creatorcontrib><creatorcontrib>Cavalleri, A</creatorcontrib><creatorcontrib>Colpi, M</creatorcontrib><creatorcontrib>Conklin, J</creatorcontrib><creatorcontrib>Cornish, N</creatorcontrib><creatorcontrib>Danzmann, K</creatorcontrib><creatorcontrib>DeBra, D</creatorcontrib><creatorcontrib>L Di Fiore</creatorcontrib><creatorcontrib>M Diaz Aguilo</creatorcontrib><creatorcontrib>Diepholz, I</creatorcontrib><creatorcontrib>Dolesi, R</creatorcontrib><creatorcontrib>Dotti, M</creatorcontrib><creatorcontrib>G Fernández Barranco</creatorcontrib><creatorcontrib>Ferraioli, L</creatorcontrib><creatorcontrib>Finetti, N</creatorcontrib><creatorcontrib>Fitzsimons, E</creatorcontrib><creatorcontrib>Galeazzi, F</creatorcontrib><creatorcontrib>Garcia, A</creatorcontrib><creatorcontrib>Giardini, D</creatorcontrib><creatorcontrib>Gibert, F</creatorcontrib><creatorcontrib>Grimani, C</creatorcontrib><creatorcontrib>Haiman, Z</creatorcontrib><creatorcontrib>Halloin, H</creatorcontrib><creatorcontrib>Heinzel, G</creatorcontrib><creatorcontrib>Hewitson, M</creatorcontrib><creatorcontrib>Hogan, C</creatorcontrib><creatorcontrib>Hornstrup, A</creatorcontrib><creatorcontrib>Hoyle, C D</creatorcontrib><creatorcontrib>Hughes, S</creatorcontrib><creatorcontrib>Kalogera, V</creatorcontrib><creatorcontrib>Karnesis, N</creatorcontrib><creatorcontrib>Killow, C</creatorcontrib><creatorcontrib>Kochkina, E</creatorcontrib><creatorcontrib>Korsakova, N</creatorcontrib><creatorcontrib>Larson, S</creatorcontrib><creatorcontrib>Livas, J</creatorcontrib><creatorcontrib>Lloro, I</creatorcontrib><creatorcontrib>Maghami, P</creatorcontrib><creatorcontrib>Marsh, T</creatorcontrib><creatorcontrib>Mateos, I</creatorcontrib><creatorcontrib>Mayer, L</creatorcontrib><creatorcontrib>McKenzie, K</creatorcontrib><creatorcontrib>Merkowitz, S</creatorcontrib><creatorcontrib>Miller, C</creatorcontrib><creatorcontrib>Mitryk, S</creatorcontrib><creatorcontrib>Moerschell, J</creatorcontrib><creatorcontrib>Mohanty, S</creatorcontrib><creatorcontrib>Monsky, A</creatorcontrib><creatorcontrib>Mueller, G</creatorcontrib><creatorcontrib>Müller, V</creatorcontrib><creatorcontrib>Nelemans, G</creatorcontrib><creatorcontrib>Nicolodi, D</creatorcontrib><creatorcontrib>Nissanke, S</creatorcontrib><creatorcontrib>Nofrarias, M</creatorcontrib><creatorcontrib>Ohme, F</creatorcontrib><creatorcontrib>Otto, M</creatorcontrib><creatorcontrib>Perreur-Lloyd, M</creatorcontrib><creatorcontrib>Plagnol, E</creatorcontrib><creatorcontrib>Prat, P</creatorcontrib><creatorcontrib>Reiche, J</creatorcontrib><creatorcontrib>Richstone, D</creatorcontrib><creatorcontrib>Robertson, D</creatorcontrib><creatorcontrib>Rubbo, L</creatorcontrib><creatorcontrib>Schlamminger, S</creatorcontrib><creatorcontrib>Schütze, D</creatorcontrib><creatorcontrib>Shah, S</creatorcontrib><creatorcontrib>Sheard, B</creatorcontrib><creatorcontrib>Spector, A</creatorcontrib><creatorcontrib>Stanga, R</creatorcontrib><creatorcontrib>Stebbins, R</creatorcontrib><creatorcontrib>Stede, G</creatorcontrib><creatorcontrib>Steier, F</creatorcontrib><creatorcontrib>Sumner, T</creatorcontrib><creatorcontrib>Sun, K -X</creatorcontrib><creatorcontrib>Thorpe, I</creatorcontrib><creatorcontrib>Tröbs, M</creatorcontrib><creatorcontrib>Tinto, M</creatorcontrib><creatorcontrib>H -B Tu</creatorcontrib><creatorcontrib>Vetrugno, D</creatorcontrib><creatorcontrib>Wang, Y</creatorcontrib><creatorcontrib>Wanner, G</creatorcontrib><creatorcontrib>Ward, H</creatorcontrib><creatorcontrib>Ware, B</creatorcontrib><creatorcontrib>Wass, P</creatorcontrib><creatorcontrib>Weber, W J</creatorcontrib><creatorcontrib>Y Yu</creatorcontrib><creatorcontrib>Zweifel, P</creatorcontrib><title>The Gravitational Universe</title><title>arXiv.org</title><description>The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it possible to trace the history of black holes across all stages of galaxy evolution, and at the same time constrain any deviation from the Kerr metric of General Relativity. eLISA will be the first ever mission to study the entire Universe with gravitational waves. eLISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the early processes at TeV energies, has guaranteed sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales around singularities and black holes, all the way to cosmological dimensions.</description><subject>Big bang cosmology</subject><subject>Black holes</subject><subject>Cosmology</subject><subject>Electromagnetic radiation</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Gravitation</subject><subject>Gravitational waves</subject><subject>Ionization</subject><subject>Milky Way Galaxy</subject><subject>Relativity</subject><subject>Singularities</subject><subject>Stellar evolution</subject><subject>Universe</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNpjYuA0MjY21LUwMTLiYOAtLs4yMDAwMjM3MjU15mSQCslIVXAvSizLLEksyczPS8xRCM3LLEstKk7lYWBNS8wpTuWF0twMym6uIc4eugVF-YWlqcUl8Vn5pUVAHcXxRgYWpkZGhsaWhsbEqQIAzUgq6A</recordid><startdate>20130524</startdate><enddate>20130524</enddate><creator>Audley, H</creator><creator>Auger, G</creator><creator>Babak, S</creator><creator>Baker, J</creator><creator>Barausse, E</creator><creator>Barke, S</creator><creator>Benacquista, M</creator><creator>Bender, P L</creator><creator>Berti, E</creator><creator>Binétruy, P</creator><creator>Bogenstahl, J</creator><creator>Bonvin, C</creator><creator>Brossard, J</creator><creator>Caprini, C</creator><creator>Cavalleri, A</creator><creator>Colpi, M</creator><creator>Conklin, J</creator><creator>Cornish, N</creator><creator>Danzmann, 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E ; Binétruy, P ; Bogenstahl, J ; Bonvin, C ; Brossard, J ; Caprini, C ; Cavalleri, A ; Colpi, M ; Conklin, J ; Cornish, N ; Danzmann, K ; DeBra, D ; L Di Fiore ; M Diaz Aguilo ; Diepholz, I ; Dolesi, R ; Dotti, M ; G Fernández Barranco ; Ferraioli, L ; Finetti, N ; Fitzsimons, E ; Galeazzi, F ; Garcia, A ; Giardini, D ; Gibert, F ; Grimani, C ; Haiman, Z ; Halloin, H ; Heinzel, G ; Hewitson, M ; Hogan, C ; Hornstrup, A ; Hoyle, C D ; Hughes, S ; Kalogera, V ; Karnesis, N ; Killow, C ; Kochkina, E ; Korsakova, N ; Larson, S ; Livas, J ; Lloro, I ; Maghami, P ; Marsh, T ; Mateos, I ; Mayer, L ; McKenzie, K ; Merkowitz, S ; Miller, C ; Mitryk, S ; Moerschell, J ; Mohanty, S ; Monsky, A ; Mueller, G ; Müller, V ; Nelemans, G ; Nicolodi, D ; Nissanke, S ; Nofrarias, M ; Ohme, F ; Otto, M ; Perreur-Lloyd, M ; Plagnol, E ; Prat, P ; Reiche, J ; Richstone, D ; Robertson, D ; Rubbo, L ; Schlamminger, S ; Schütze, D ; Shah, S ; Sheard, B ; Spector, A ; Stanga, R ; Stebbins, R ; Stede, G ; Steier, F ; Sumner, T ; Sun, K -X ; Thorpe, I ; Tröbs, M ; Tinto, M ; H -B Tu ; Vetrugno, D ; Wang, Y ; Wanner, G ; Ward, H ; Ware, B ; Wass, P ; Weber, W J ; Y Yu ; Zweifel, P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20852213913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Big bang cosmology</topic><topic>Black holes</topic><topic>Cosmology</topic><topic>Electromagnetic radiation</topic><topic>Galactic evolution</topic><topic>Galaxies</topic><topic>Gravitation</topic><topic>Gravitational waves</topic><topic>Ionization</topic><topic>Milky Way Galaxy</topic><topic>Relativity</topic><topic>Singularities</topic><topic>Stellar evolution</topic><topic>Universe</topic><toplevel>online_resources</toplevel><creatorcontrib>Audley, H</creatorcontrib><creatorcontrib>Auger, G</creatorcontrib><creatorcontrib>Babak, S</creatorcontrib><creatorcontrib>Baker, 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H</creatorcontrib><creatorcontrib>Ware, B</creatorcontrib><creatorcontrib>Wass, P</creatorcontrib><creatorcontrib>Weber, W J</creatorcontrib><creatorcontrib>Y Yu</creatorcontrib><creatorcontrib>Zweifel, P</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Audley, H</au><au>Auger, G</au><au>Babak, S</au><au>Baker, J</au><au>Barausse, E</au><au>Barke, S</au><au>Benacquista, M</au><au>Bender, P L</au><au>Berti, E</au><au>Binétruy, P</au><au>Bogenstahl, J</au><au>Bonvin, C</au><au>Brossard, J</au><au>Caprini, C</au><au>Cavalleri, A</au><au>Colpi, M</au><au>Conklin, J</au><au>Cornish, N</au><au>Danzmann, K</au><au>DeBra, D</au><au>L Di Fiore</au><au>M Diaz Aguilo</au><au>Diepholz, I</au><au>Dolesi, R</au><au>Dotti, M</au><au>G Fernández Barranco</au><au>Ferraioli, L</au><au>Finetti, N</au><au>Fitzsimons, E</au><au>Galeazzi, F</au><au>Garcia, A</au><au>Giardini, D</au><au>Gibert, F</au><au>Grimani, C</au><au>Haiman, Z</au><au>Halloin, H</au><au>Heinzel, G</au><au>Hewitson, M</au><au>Hogan, C</au><au>Hornstrup, A</au><au>Hoyle, C D</au><au>Hughes, S</au><au>Kalogera, V</au><au>Karnesis, N</au><au>Killow, C</au><au>Kochkina, E</au><au>Korsakova, N</au><au>Larson, S</au><au>Livas, J</au><au>Lloro, I</au><au>Maghami, P</au><au>Marsh, T</au><au>Mateos, I</au><au>Mayer, L</au><au>McKenzie, K</au><au>Merkowitz, S</au><au>Miller, C</au><au>Mitryk, S</au><au>Moerschell, J</au><au>Mohanty, S</au><au>Monsky, A</au><au>Mueller, G</au><au>Müller, V</au><au>Nelemans, G</au><au>Nicolodi, D</au><au>Nissanke, S</au><au>Nofrarias, M</au><au>Ohme, F</au><au>Otto, M</au><au>Perreur-Lloyd, M</au><au>Plagnol, E</au><au>Prat, P</au><au>Reiche, J</au><au>Richstone, D</au><au>Robertson, D</au><au>Rubbo, L</au><au>Schlamminger, S</au><au>Schütze, D</au><au>Shah, S</au><au>Sheard, B</au><au>Spector, A</au><au>Stanga, R</au><au>Stebbins, R</au><au>Stede, G</au><au>Steier, F</au><au>Sumner, T</au><au>Sun, K -X</au><au>Thorpe, I</au><au>Tröbs, M</au><au>Tinto, M</au><au>H -B Tu</au><au>Vetrugno, D</au><au>Wang, Y</au><au>Wanner, G</au><au>Ward, H</au><au>Ware, B</au><au>Wass, P</au><au>Weber, W J</au><au>Y Yu</au><au>Zweifel, P</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The Gravitational Universe</atitle><jtitle>arXiv.org</jtitle><date>2013-05-24</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it possible to trace the history of black holes across all stages of galaxy evolution, and at the same time constrain any deviation from the Kerr metric of General Relativity. eLISA will be the first ever mission to study the entire Universe with gravitational waves. eLISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the early processes at TeV energies, has guaranteed sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales around singularities and black holes, all the way to cosmological dimensions.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2013-05 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_proquest_journals_2085221391 |
| source | Free E- Journals |
| subjects | Big bang cosmology Black holes Cosmology Electromagnetic radiation Galactic evolution Galaxies Gravitation Gravitational waves Ionization Milky Way Galaxy Relativity Singularities Stellar evolution Universe |
| title | The Gravitational Universe |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-09T21%3A54%3A05IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=The%20Gravitational%20Universe&rft.jtitle=arXiv.org&rft.au=Audley,%20H&rft.date=2013-05-24&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2085221391%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2085221391&rft_id=info:pmid/&rfr_iscdi=true |