Gravitational Waves and Coalescing Black Holes
Gravitation is a manifestation of the space-time curvature and gravitational waves aredistortions traveling through the fabric of space-time. Scientists have tried to detectgravitational waves for decades, but the first direct detection of gravitational waves andthe first observation of a binary bla...
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KTH, Skolan för teknikvetenskap (SCI)
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ndltd-UPSALLA1-oai-DiVA.org-kth-2108492017-07-07T05:31:03ZGravitational Waves and Coalescing Black HolesengJoanna, EkehultKarpinska, AnnaKTH, Skolan för teknikvetenskap (SCI)KTH, Skolan för teknikvetenskap (SCI)2017Engineering and TechnologyTeknik och teknologierGravitation is a manifestation of the space-time curvature and gravitational waves aredistortions traveling through the fabric of space-time. Scientists have tried to detectgravitational waves for decades, but the first direct detection of gravitational waves andthe first observation of a binary black hole merger was made in 2015. The purpose ofthis report is to introduce General Relativity and binary black holes and to calculate thetime to coalescence of two back holes with circular or elliptical orbits. We find that abinary black hole in an elliptical orbit with large eccentricity coalesces faster than in acircular orbit. Student thesisinfo:eu-repo/semantics/bachelorThesistexthttp://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-210849application/pdfinfo:eu-repo/semantics/openAccess |
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English |
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Engineering and Technology Teknik och teknologier |
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Engineering and Technology Teknik och teknologier Joanna, Ekehult Karpinska, Anna Gravitational Waves and Coalescing Black Holes |
description |
Gravitation is a manifestation of the space-time curvature and gravitational waves aredistortions traveling through the fabric of space-time. Scientists have tried to detectgravitational waves for decades, but the first direct detection of gravitational waves andthe first observation of a binary black hole merger was made in 2015. The purpose ofthis report is to introduce General Relativity and binary black holes and to calculate thetime to coalescence of two back holes with circular or elliptical orbits. We find that abinary black hole in an elliptical orbit with large eccentricity coalesces faster than in acircular orbit. |
author |
Joanna, Ekehult Karpinska, Anna |
author_facet |
Joanna, Ekehult Karpinska, Anna |
author_sort |
Joanna, Ekehult |
title |
Gravitational Waves and Coalescing Black Holes |
title_short |
Gravitational Waves and Coalescing Black Holes |
title_full |
Gravitational Waves and Coalescing Black Holes |
title_fullStr |
Gravitational Waves and Coalescing Black Holes |
title_full_unstemmed |
Gravitational Waves and Coalescing Black Holes |
title_sort |
gravitational waves and coalescing black holes |
publisher |
KTH, Skolan för teknikvetenskap (SCI) |
publishDate |
2017 |
url |
http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-210849 |
work_keys_str_mv |
AT joannaekehult gravitationalwavesandcoalescingblackholes AT karpinskaanna gravitationalwavesandcoalescingblackholes |
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1718492286578327552 |