Session

Tidal Disruption Events

12 Nov 2026, 13:30
Auditorium (Haus der Astronomie)

Auditorium

Haus der Astronomie

Königstuhl 17 69117 Heidelberg

Presentation materials

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  1. Jane Dai
    12/11/2026, 13:30
    Talks
  2. Dr Clément Bonnerot (University of Birmingham)
    12/11/2026, 14:00
    Tidal Disruption Events
    Talks

    Tidal disruption events occur when a star ventures too close to a supermassive black hole and is torn apart by tidal forces, producing a luminous flare as the stellar debris fuels the compact object. Interpreting observations requires connecting the complex hydrodynamics of the disrupted debris to the processes that shape the emerging radiation. In this talk, I will present a suite of...

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  3. Simona Pacuraru (University of Birmingham)
    12/11/2026, 14:20
    Tidal Disruption Events
    Talks

    A tidal disruption event (TDE) occurs when a star is torn apart by the strong tidal pull of a supermassive black hole. The disruption results in the formation of an elongated stream of gas which cools down adiabatically due to the tidal stretching. As the temperature drops, the gas is expected to undergo chemical processes, which release thermal energy into the stream, potentially affecting...

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  4. Brenna Mockler
    12/11/2026, 15:30
  5. Chun-Ming Yip (GSI Helmholtzzentrum für Schwerionenforschung GmbH (GSI))
    12/11/2026, 16:00
    Talks

    The kilonova AT2017gfo has demonstrated that neutron-star mergers indeed are astrophysical sites of the r-process, yet the detailed properties of its various ejecta components remain poorly understood. Numerical simulations of neutron star mergers, including all relevant physics ingredients and encompassing both the dynamical merger phase and the subsequent remnant evolution, are essential for...

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  6. Shane Davis (University of Virginia)
    12/11/2026, 16:20
    Tidal Disruption Events
    Talks

    I will present results from recent research by myself and collaborators to study the disruption and fallback accretion during tidal disruption events. Using the state-of-the-art Athena++ and AthenaK codes, we solve the radiation transfer equation to accurately model the radiation forces, which play a key role in these sources that commonly reach super-Eddington fallback rates. I will...

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