NASA’s infra-red observatory Spitzer has recently observed the flare from gigantic binary черна дупка system OJ 287, within the estimated time interval predicted by the model developed by astrophysicists. This observation has tested different aspects of General Relativity, the “No-hair theorem”, and proved that OJ 287 is indeed a source of infra-red Гравитационни вълни.
- ОВ 287 galaxy, situated in Cancer constellation 3.5 billion light years away from Earth, has two черни дупки – the larger one with over 18 billion times the mass of the Sun and orbiting this is a smaller черна дупка with about 150 million times the solar mass, and they form a binary черна дупка system. While orbiting the larger one, the smaller черна дупка crashes through the enormous accretion disk of gas and dust surrounding its larger companion, creating a flash of light brighter than a trillion stars.
По-малките черна дупка collides with the accretion disk of the larger one twice in every twelve years. However, due to its irregular oblong orbit (called quasi-Keplarian in the mathematical terminology, as shown in the figure below), the flares can appear at different times – sometimes as little as one year apart; other times, as much as 10 years apart (1). Several attempts to model the orbit and predicting when flares would happen were unsuccessful until in 2010, when astrophysicists created a model that could predict their occurrence with an error of about one to three weeks. The accuracy of the model was demonstrated by predicting the appearance of a flare in December 2015 to within three weeks.
Another important piece of information that went into the making of a successful theory of binary черна дупка system OJ 287 is the fact that supermassive черни дупки can be sources of гравитационни вълни – which has been established after the experimental observation of the гравитационни вълни in 2016, produced during the merging of two supermassive черни дупки. OJ 287 has been predicted to be the source of infra-red гравитационни вълни (2).
In 2018, a group of astrophysicists provided an even more detailed model, and claimed to be able to predict the timing of future flares to within few hours (3). According to this model, the next flare would occur on July 31, 2019 and the time was predicted with an error of 4.4 hours. It also predicted the brightness of the impact-induced flare to take place during that event. The event was captured and confirmed by NASA’s Spitzer Space Telescope (4), which retired in January 2020. To observe the predicted event, Spitzer was our only hope since this flare could not be seen by any other telescope on the ground or in Earth’s orbit, as the Sun was in Cancer constellation with OJ 287 and Earth being on opposite sides of it. This observation also proved that OJ 287 emits гравитационни вълни in the infra-red wavelength, as predicted. According to this proposed theory the impact-induced flare from OJ 287 is expected to take place in 2022.
Наблюденията на тези изригвания поставят ограничение върху „Няма теорема за косата” (5,6) which states that while черни дупки don’t have true surfaces, there is a boundary around them beyond which nothing – not even light – can escape. This boundary is called the event horizon. This theorem also postulates that the matter which forms a black-hole or is falling into it “disappears” behind the черна дупка event horizon and is therefore permanently inaccessible to external observers, suggesting that черни дупки have “no hair”. One immediate consequence of the theorem is that the черни дупки can be characterized completely with their mass, electric charge and intrinsic spin. According to some scientists, this outer edge of the black-hole, i.e. the event horizon, could be bumpy or irregular, thus contradicting the “No hair theorem”. However, if one has to prove the correctness of the “No hair theorem”, the only plausible explanation is that the uneven mass distribution of the large black-hole would distort the space around it in such a manner that it would lead to a change of path of the smaller черна дупка, and in turn change the timing of the black hole’s collision with the accretion disk on that particular orbit, thus causing a change in the time of appearance of the flares observed.
Както може да се очаква, черни дупки are hard to probe. Hence, as we move forward, many more experimental observations regarding черна дупка interactions, with the surroundings as well as with other black holes, are to be studied before one can confirm the validity of the “No hair theorem”.
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Литература:
- Валтонен В., Зола С., и др. 2016 г., „Завъртане на първичната черна дупка в OJ287, определено от стогодишния изригване на общата относителност“, Astrophys. J. Lett. 819 (2016) № 2, L37. DOI: https://doi.org/10.3847/2041-8205/819/2/L37
- Abbott BP., и др. 2016. (LIGO Scientific Collaboration and Virgo Collaboration), „Наблюдение на гравитационни вълни от сливане на двоична черна дупка“, Phys. преп. Лет. 116, 061102 (2016). DOI: https://doi.org/10.1103/PhysRevLett.116.061102
- Дей Л., Валтонен М. Дж., Гопакумар А. и др 2018. „Удостоверяване на присъствието на релативистична масивна двоична черна дупка в OJ 287, използвайки нейното столетно изригване на общата относителност: подобрени орбитални параметри“, Астрофизис. J. 866, 11 (2018). DOI: https://doi.org/10.3847/1538-4357/aadd95
- Лейн С., Дей Л., и др 2020. „Наблюдения на Спицър на прогнозирания пламък на Eddington от Blazar OJ 287“. Astrophysical Journal Letters, кн. 894, № 1 (2020). DOI: https://doi.org/10.3847/2041-8213/ab79a4
- Gürlebeck, N., 2015. „Теорема без косъм за черни дупки в астрофизични среди“, Физически писма преглед 114, 151102 (2015). DOI: https://doi.org/10.1103/PhysRevLett.114.151102
- Хокинг Стивън У. и др. 2016. Мека коса върху черните дупки. https://arxiv.org/pdf/1601.00921.pdf
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