重力波、黑洞併合與中子星併合


Seminar:- Gravitational Waves, Merging Black Holes and Merging Binary Neutron Stars - 2017 Nobel Prize in Physics

The detection of gravitational waves from the mergers of binary black holes by the Advanced LIGO detectors has provided a first glimpse on the most energetic phenomena in the Universe. On 14 September 2015, the advanced Laser Interferometer Gravitational Wave Observatory (aLIGO) at the very beginning of its operation observed the merger of a binary black hole pair of masses 36 and 29 times that of the Sun. This event initiated the era of observational gravitational wave astronomy and allowed probing strong field General Relativity theory, the population of stellar remnants including black holes as well as finally confirming a 100-year-old prediction of the existence of gravitational waves by Einstein. Over the last two years, two more events and one candidate events of binary black hole mergers have been observed, enriching our knowledge of these phenomena greatly and promising even more as aLIGO and new detector are added and upgraded. These discoveries led to the 2017 Nobel Prize in Physics.

Recently on 17 August 2017, LIGO and Virgo made the first detection of a binary neutron star merger, GW170817. Two seconds later, an associated gamma-ray burst (GRB) was detected by Fermi and INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory) satellites, GRB 170817A. Soon after sunset in Chile, the 1-meter Swope telescope at Las Campanas Observatory discovered the optical counterpart, Swope Supernova Survey 2017a (SSS17a). Observations taken over the next several weeks extended the range of frequencies observed and 30 different telescopes and detectors following the relic radiation. With the electromagnetic data, we are able to say that GW170817 came from the merger of a binary neutron star system. These data show that a significant amount of r-process materials were generated and ejected in the merger - a so-called "kilonova" - providing enough material to solve the question of where the majority of r-process (heavier) elements are created. Examining the host galaxy, we find that the progenitor system was likely several Giga-years old. This data-rich event is just the beginning. GW170817 and SSS17a herald the beginning of a new era of astronomy.

In this talk, the speaker will tell the tale of these discoveries and their implications. 
 
時間:2017.11.14(二) 15:00 ~ 16:30
地點:香港科技大學 李兆基校園 盧家驄薈萃樓 高研院演講廳
講者:Prof George F Smoot(香港科技大學 高等研究院 趙氏廷箴懷芳基金會教授 首席物理教授)
語言:英語

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此活動由香港科技大學 賽馬會高等研究院主辦。

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