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Andrea Perali (University of Camerino)16/09/2025, 09:00
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Jan Harms (Gran Sasso Science Institute)16/09/2025, 09:15
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Gianluca Polenta (ASI)16/09/2025, 09:40
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Shyama Narendranath (ISRO)16/09/2025, 10:05
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Luigi Cacciapuoti (ESA)16/09/2025, 11:00
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Flavio Travasso (University of Camerino)16/09/2025, 11:30
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Amir Khan (ETH Zurich)16/09/2025, 12:00
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Friedrich Röpke (Ruprecht-Karls University Heidelberg)16/09/2025, 14:30
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David Vartanyan (Carnegie Observatories)16/09/2025, 15:00
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Francesco Iacovelli (Johns Hopkins University)16/09/2025, 15:30
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Jasbir Singh (Istituto Nazionale di Astrofisica (INAF))17/09/2025, 09:00
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Xin Li (Nanjing University)17/09/2025, 09:30
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Fabio Rigamonti (Istituto Nazionale di Astrofisica (INAF))17/09/2025, 10:00
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Shreevathsa Subrahmanya (University of Hamburg)17/09/2025, 11:00
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Andrea Perali (University of Camerino), Meenakshi Sharma (MPG CPFS)17/09/2025, 11:20
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Mayana Teloi (University of Liège)17/09/2025, 11:40
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Ilaria Caravella (GSSI), Jan Harms (Gran Sasso Science Institute)17/09/2025, 12:00
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Ajith Parameswaran (ICTS)17/09/2025, 14:30
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Giuliano Iorio (ICCUB)17/09/2025, 15:10
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Alexey Bobrick (Monash University)17/09/2025, 15:35
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Lion Krischer (Mondaic Ltd)17/09/2025, 16:30
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Heiner Igel (LMU)17/09/2025, 16:55
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Sheng Wang (ETH Zurich)17/09/2025, 17:20
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Carlo Albanese (Telespazio)18/09/2025, 09:00
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Alexey Martinov (Sab Aerospace)18/09/2025, 09:30
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18/09/2025, 10:00
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Alessia Franchini (Milano Bicocca)18/09/2025, 14:30
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Elisabeth Keppler (SISSA)18/09/2025, 14:55
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Erwan Quintin (ESA)18/09/2025, 15:25
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Caitlin Ahrens (NASA GSFC)18/09/2025, 16:30
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Hrvoje Tkalcic (ANU)18/09/2025, 16:55
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Luca De Siena (University of Bologna)18/09/2025, 17:20
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Giuliano Iorio (Istituto Nazionale di Astrofisica (INAF))
The first direct detection of gravitational waves on 14 September 2015, from the merger of two stellar-mass black holes, marked a milestone in astrophysics and inaugurated the era of multi-messenger astronomy. In the decade since, LVK interferometers have detected hundreds of mergers involving binary black holes, binary neutron stars, and mixed systems, offering valuable insights into compact...
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Dr Shreevathsa Chalathadka Subrahmanya (University of Hamburg)
One of the key components of the payload of the Lunar Gravitational-Wave Antenna is the inertial sensor, which measures the differential motion between the lunar surface and the inertial mass. To detect gravitational waves, the inertial mass motion must be read out with sub-femtometer precision.
In this talk, I introduce a laser interferometric displacement sensing scheme called heterodyne...
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Elisabeth Keppler (SISSA)
When a star orbits close enough to a black hole and interacts with its tidal forces, disruption may happen. The stellar debris accretes along the orbital plane to form a disk, which is then accelerated and acquires energy enough to form a jet. A luminous flare of photons in X-ray, optical, infrared and radio is observed, which takes the name of Tidal Disruption Event (TDE).
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TDEs are already a... -
Ferdinando Patat (ESO)
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Dr Alexey Bobrick (Monash University)
The decihertz gravitational wave window enabled by LGWA will provide a unique view of the shortest-period compact binaries and their immediate outcomes, otherwise inaccessible with current instruments. For double white dwarfs and white dwarf-neutron star binaries, LGWA will constrain the physics of the late pre-merger evolution and, through multi-messenger observations, provide the first...
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