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Seminar Vật lý lý thuyết và Vật lý tính toán:
Tên báo cáoHawking fluxes and Anomalies in Rotating Regular Black Holes with a Time-Delay
Người trình bàyDr. Shingo Takeuchi
Cơ quanThe Institute for Fundamental Study (IF), Naresuan University, Phitsanulok 99 Moo 9 Tambol Taephoe, Amphur Muang, Phisanulok, 65000, Thailand
NgàyThứ Ba, 29-11-2016
Giờ10:00 AM
Địa điểmPhòng 202 (Thư viện), Viện Vật lý, 10 Đào Tấn, Ba Đình, Hà Nội
Tóm tắtAlthough derivation of Hawking fluxes has been already performed around 1974 by Hawking based on the pair-creation in the vicinity of the near-horizon region, around 2005 Hawking fluxes have been again derived based on the anomaly-free condition [1,2]. This way would be very intriguing, because it will suggest the following two points:

1) Hawking fluxes might be the fluxes appearing as the quantum tunneling in order to compensate for the deficit of outgoing modes on the horizon so as to be anomaly-free at the semi-classical level.

2) A picture in which Hawking fluxes and Bekenstein-Hawking entropy are drown uniformly.

In this seminar, based on my study as in the title, I would like to introduce the way for the derivation of Hawking fluxes based on anomaly-free condition and the physics mentioned above.

Further I will give a comment about which models proposed in [3] as the regular black hole with a time-delay are physically consistent. This would be beneficial for the future works based on the regular black holes with a time-delay in [3].

[1] S. P. Robinson and F. Wilczek, gr-qc/0502074.

[2] S. Iso, H. Umetsu and F. Wilczek, hep-th/0602146.

[3] T. De Lorenzo, A. Giusti and S. Speziale, arXiv:1510.08828.
Người chủ trìNguyễn Anh Kỳ