{"title":"引力波作为独特的超宽带过程","authors":"L. Chernogor, Oleg V. Lazorenko","doi":"10.1109/UWBUSIS.2016.7724148","DOIUrl":null,"url":null,"abstract":"The results of system spectral analysis of the unique registration of the gravitational waves generated by a binary black hole merger were proposed. On September 14, 2015 at 09:50:45 UTC two detectors of the Laser Interferometer Gravitational-Wave Observatory placed in the United States simultaneously observed a transient gravitational-wave signal. These were the first direct detection of gravitational waves and the first direct observation of a binary black hole system merging to form a single black hole. Using the system spectral analysis method, the time-frequency structure of the gravitational wave signal was investigated in detail. This signal was found to be classified as an ultra-wideband process with changing mean frequency.","PeriodicalId":423697,"journal":{"name":"2016 8th International Conference on Ultrawideband and Ultrashort Impulse Signals (UWBUSIS)","volume":"15 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Gravitational waves as the unique ultra-wideband process\",\"authors\":\"L. Chernogor, Oleg V. Lazorenko\",\"doi\":\"10.1109/UWBUSIS.2016.7724148\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The results of system spectral analysis of the unique registration of the gravitational waves generated by a binary black hole merger were proposed. On September 14, 2015 at 09:50:45 UTC two detectors of the Laser Interferometer Gravitational-Wave Observatory placed in the United States simultaneously observed a transient gravitational-wave signal. These were the first direct detection of gravitational waves and the first direct observation of a binary black hole system merging to form a single black hole. Using the system spectral analysis method, the time-frequency structure of the gravitational wave signal was investigated in detail. This signal was found to be classified as an ultra-wideband process with changing mean frequency.\",\"PeriodicalId\":423697,\"journal\":{\"name\":\"2016 8th International Conference on Ultrawideband and Ultrashort Impulse Signals (UWBUSIS)\",\"volume\":\"15 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-09-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2016 8th International Conference on Ultrawideband and Ultrashort Impulse Signals (UWBUSIS)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/UWBUSIS.2016.7724148\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2016 8th International Conference on Ultrawideband and Ultrashort Impulse Signals (UWBUSIS)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/UWBUSIS.2016.7724148","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Gravitational waves as the unique ultra-wideband process
The results of system spectral analysis of the unique registration of the gravitational waves generated by a binary black hole merger were proposed. On September 14, 2015 at 09:50:45 UTC two detectors of the Laser Interferometer Gravitational-Wave Observatory placed in the United States simultaneously observed a transient gravitational-wave signal. These were the first direct detection of gravitational waves and the first direct observation of a binary black hole system merging to form a single black hole. Using the system spectral analysis method, the time-frequency structure of the gravitational wave signal was investigated in detail. This signal was found to be classified as an ultra-wideband process with changing mean frequency.