logo

Tidal Disruption Events: A New Black Hole Census

Sector: Power Generation (CCGT) • Location: Israel

Source: EU Funding & Tenders Portal

Project
Ended

Massive black holes (MBHs) are key players in high energy astrophysics, galaxy formation and evolution, and astroparticle physics. Despite their centrality to astronomy, we still cannot answer basic questions about MBHs. What are their origins? How have they grown over cosmic time? What are their current demographics? To answer these questions, the project will turn tidal disruption events (TDEs)

Status
Closed
Sector
Power Generation (CCGT), Education
Location
Israel
Updated
22 Jul 2026
Source
EU Funding & Tenders Portal

ConstructChat

Ask ConstructChat about Tidal Disruption Events: A New Black Hole Census

Pick a question to edit it, or write your own.

First answer free · no account

I am a

Project Information FAQ

Project Information

3 Q
The project “Tidal Disruption Events: A New Black Hole Census” is an infrastructure initiative in the Power Generation (CCGT) sector, located in Israel. Taiyo aggregates data on it from EU Funding & Tenders Portal.

Participants

Not available for this record.

Status

Original status

ended

Taiyo status

Closed

Taiyo last update

2026-07-22

Contact

Not available for this record.

Description

Description

Massive black holes (MBHs) are key players in high energy astrophysics, galaxy formation and evolution, and astroparticle physics. Despite their centrality to astronomy, we still cannot answer basic questions about MBHs. What are their origins? How have they grown over cosmic time? What are their current demographics? To answer these questions, the project will turn tidal disruption events (TDEs) from curiosities into reliable probes of MBH parameters. A TDE occurs when an unlucky star passes too close to a MBH and is ripped apart by tidal forces. The ensuing fallback of debris powers a highly luminous, potentially multimessenger flare. TDEs are, in principle, ideal probes of MBH properties. Unlike standard techniques for measuring MBHs, TDEs (i) happen in all galaxies, (ii) are visible to cosmological distances, and (iii) involve very few free parameters. But the theoretical picture of TDEs remains confused, as the large dynamic range of TDEs has prevented ab initio simulations to determine how tidal debris evolves and radiates. At present, there is no consensus on the geometry or even the power source of observed TDE flares, making robust parameter estimation impossible. I will solve these open theoretical questions, capitalizing on my recent pilot study that for the first time ever simulated a typical, first-principles TDE. This project will deliver (a) first-principles simulations of the evolution and emission of TDEs; (b) idealized but accurate models of TDE light curves and spectra suitable for parameter estimation; (c) a first-ever sample of MBH parameters derived from fitting ab initio models to TDE observations. I will use these results to sidestep the limitations of other MBH measurement techniques and to place unique constraints on the formation and growth history of the smallest MBHs. This work is urgently needed in light of upcoming all-sky surveys such as ULTRASAT and LSST, which will expand the TDE sample from dozens to thousands in the mid-2020s.

Location

Country

Israel

Source

Source

EU Funding & Tenders Portal

URL

More Details

Record type

Project

Sector

Power Generation (CCGT), Education

Article published date

2026-02-15

More on this project

Research

Free account

View all details

You are reading the public part. A free account opens the rest:

  • Every detail on this project
  • News and media coverage
  • Technical research
View all details

Free account · no card · lands you back on this project