High accuracy measurement of gravitational wave back-reaction in the OJ287 black hole binary
作者: Mauri J. ValtonenL. DeyR. HudecS. ZolaA. GopakumarS. MikkolaS. CipriniK. MatsumotoK. SadakaneM. KidgerK. GazeasK. NilssonA. BerdyuginV. PiirolaH. JermakK.S. BaliyanD. E. ReichartD. B. CatonS. Haque
作者单位: 11 Department of Physics and Astronomy , University of Turku , Väisäläntie 20 , FIN-21500 , Kaarina , Finland email: mvaltonen2001@yahoo.com
2 2 Finnish Centre for Astronomy with ESO , University of Turku , Väisäläntie 20 , FIN-21500 Kaarina , Finland
3 3 Department of Astronomy and Astrophysics , Tata Institute of Fundamental Research , Mumbai 400005 , India
4 4 Astronomical Institute , The Czech Academy of Sciences , 25165 Ondřejov , Czech Republic
5 5 Czech Technical University in Prague , Faculty of Electrical Engineering , Prague , Czech Republic
6 6 Astronomical Observatory , Jagiellonian University , ul. Orla 171 , Cracow PL-30-244 , Poland
7 7 Mt. Suhora Astronomical Observatory , Pedagogical University , ul. Podchorazych 2 , PL30-084 Cracow , Poland
8 8 Agenzia Spaziale Italiana (ASI) Space Science Data Center , I-00133 Roma , Italy
9 9 Istituto Nazionale di Fisica Nucleare , Sezione di Perugia ,
刊名: Proceedings of the International Astronomical Union, 2019, Vol.13 (S338), pp.29-36
来源数据库: Cambridge University Press Journal
DOI: 10.1017/S1743921318000170
原始语种摘要: Abstract Blazar OJ287 exhibits large thermal flares at least twice every 12 years. The times of these flares have been predicted successfully using the model of a quasi-Keplerian eccentric black hole binary where the secondary impacts the accretion disk of the primary, creating the thermal flares. New measurements of the historical light curve have been combined with the observations of the 2015 November/December flare to identify the impact record since year 1886, and to constrain the orbit of the binary. The orbital solution shows that the binary period, now 12.062 years, is decreasing at the rate of 36 days per century. This corresponds to an energy loss to gravitational waves that is 6.5 ± 4 % less than the rate predicted by the standard quadrupolar gravitational wave (GW) emission....
全文获取路径: Cambridge U Press  (合作)

  • gravitational 重力
  • flares 喇叭裤
  • reaction 反酌
  • quadrupolar 四极的
  • black 炭黑
  • historical 历史的
  • identify 视为同一
  • binary 二元的
  • predicted 预先计算的
  • century 世纪