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相关论文: The TDE Population from First-Principles Models of…

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We study tidal disruption events (TDEs) and compact object inspirals in nuclear star clusters (NSCs) hosting a central supermassive black hole (SMBH), focusing on their role in SMBH growth. Using the STARDISK version of the direct N-body…

星系天体物理 · 物理学 2026-02-10 Philip Cho , Kai Wu , Francesco Flammini Dotti , Taras Panamarev , Rainer Spurzem

The tidal disruption of a star by a supermassive black hole (SMBH) is a highly energetic event with consequences dependent on the degree to which the star plunges inside the SMBH's tidal sphere. We introduce a new analytic model for tidal…

高能天体物理现象 · 物理学 2015-06-11 Nicholas Stone , Re'em Sari , Abraham Loeb

Intermediate-mass black holes (IMBH) are expected to exist in globular clusters (GCs) and compact stellar systems (CSS) in general, but none have been conclusively detected. Tidal disruption events (TDEs), where a star is tidally disrupted…

星系天体物理 · 物理学 2025-06-04 Richard T. Pomeroy , Mark A. Norris

A tidal disruption event (TDE) occurs when a star passes too close to a supermassive black hole and gets torn apart by its gravitational tidal field. After the disruption, the stellar debris form an expanding gaseous stream. The morphology…

高能天体物理现象 · 物理学 2020-05-20 Andrea Sacchi , Giuseppe Lodato , Claudia Toci , Valentina Motta

Tidal disruption events\,(TDEs) provide a valuable probe in studying the dynamics of stars in the nuclear environments of galaxies. Recent observations show that TDEs are strongly overrepresented in post-starburst or "green valley"…

高能天体物理现象 · 物理学 2024-01-01 Mengye Wang , Yiqiu Ma , Qingwen Wu , Ning Jiang

Stars passing too close to a black hole can produce tidal disruption events (TDEs), when the tidal force across the star exceeds the gravitational force that binds it. TDEs have usually been discussed in relation to massive black holes that…

星系天体物理 · 物理学 2019-08-21 Giacomo Fragione , Nathan Leigh , Rosalba Perna , Bence Kocsis

Using archival SDSS multi-epoch imaging data (Stripe 82), we have searched for the tidal disruption of stars by super-massive black holes in non-active galaxies. Two candidate tidal disruption events (TDEs) are identified. They have optical…

When a star passes through the tidal disruption radius of a massive black hole (BH), it can be torn apart by the tidal force of the BH, known as the Tidal Disruption Event (TDE). Since the observed UV/optical luminosity significantly…

We constrain the recent star formation histories of the host galaxies of eight optical/UV-detected tidal disruption events (TDEs). Six hosts had quick starbursts of <200 Myr duration that ended 10 to 1000 Myr ago, indicating that TDEs arise…

星系天体物理 · 物理学 2017-03-29 K. Decker French , Iair Arcavi , Ann Zabludoff

The volumetric rate of tidal disruption events (TDEs) encodes information on the still-unknown demographics of central massive black holes (MBHs) in low-mass galaxies ($\lesssim 10^9$~M$_\odot$). Theoretical TDE rates from model galaxy…

星系天体物理 · 物理学 2024-07-16 Christian H. Hannah , Anil C. Seth , Nicholas C. Stone , Sjoert van Velzen

Once per 10,000-100,000 years, an unlucky star may experience a close encounter with a supermassive black hole (SMBH), partially or fully tearing apart the star in an exceedingly brief, bright interaction called a tidal disruption event…

We estimate the rate of tidal disruption events (TDEs) that will be detectable with future gravitational wave detectors as well as the most probable properties of these events and their possible electromagnetic counterpart. To this purpose…

高能天体物理现象 · 物理学 2021-12-08 Hugo Pfister , Martina Toscani , Thomas Hong Tsun Wong , Jane Lixin Dai , Giuseppe Lodato , Elena M. Rossi

In this paper we develop a computationally efficient, two-population, time-dependent Fokker-Plank approach in the two dimensions of energy and angular momentum to study the rates of tidal disruption events (TDEs), extreme mass ratio…

星系天体物理 · 物理学 2022-06-08 Luca Broggi , Elisa Bortolas , Matteo Bonetti , Alberto Sesana , Massimo Dotti

A tidal disruption event (TDE) occurs when a supermassive black hole disrupts a nearby passing star by tidal forces. The subsequent fallback accretion of the stellar debris results in a luminous transient outburst. Modeling the light curve…

高能天体物理现象 · 物理学 2023-03-29 Zsófia V. Kovács-Stermeczky , József Vinkó

Tidal Disruption Events (TDEs) have recently been proposed as potential probes for Population III stars. However, the properties of the accretion flow and the wind from the Pop III star TDE system are not clear. By performing radiative…

高能天体物理现象 · 物理学 2025-12-29 Yu-Heng Sheng , De-Fu Bu , Xiao-Hong Yang , Yi-Ren Chang , Liang Chen

The first generation metal-free stars, referred to as population III (Pop III) stars, are believed to be the first objects to form out of the pristine gas in the very early Universe. Pop III stars have different structures from current…

高能天体物理现象 · 物理学 2024-05-14 Rudrani Kar Chowdhury , Janet N. Y. Chang , Lixin Dai , Priyamvada Natarajan

A star completely destroyed in a tidal disruption event (TDE) ignites a luminous flare that is powered by the fallback of tidally stripped debris to a supermassive black hole (SMBH) of mass $M_{\bullet}$. We analyze two estimates for the…

Tidal disruption events (TDEs) occur when a star is disrupted by the tidal forces of a supermassive black hole (SMBH), producing bright multi-wavelength flares. Among these events, AT2020mot has so far exhibited the highest recorded optical…

A nuclear transient detected in a post-starburst galaxy or other quiescent galaxy with strong Balmer absorption is likely to be a Tidal Disruption Event (TDE). Identifying such galaxies within the planned survey footprint of the Large…

星系天体物理 · 物理学 2018-11-29 K. Decker French , Ann I. Zabludoff

The flare produced when a star is tidally disrupted by a supermassive black hole holds potential as a diagnostic of both the black hole mass and the star mass. We propose a new method to realize this potential based upon a physical model of…

高能天体物理现象 · 物理学 2020-12-02 Taeho Ryu , Julian Krolik , Tsvi Piran