💥UPSC 2026, 2027 UAP Mentorship November Batch

Gravitational Wave Observations

Gamma-Ray Bursts from Black Hole ‘Morsels’ could expose Quantum Gravity

Why in the News?

A recent theoretical study (accepted in Nuclear Physics B, August 2025) introduces the idea of “black hole morsels”, tiny, asteroid-mass micro-black holes possibly formed during black hole mergers.

What are Gamma-Ray Bursts (GRBs)?

  • Overview: They are extremely energetic cosmic explosions that emit intense bursts of gamma radiation, the highest-energy form of electromagnetic waves.
  • Discovery: First detected in the late 1960s by U.S. Vela satellites, initially built to monitor nuclear tests.
  • Duration-Based Classification:
    • Short GRBs: Lasting <2 seconds, typically formed by merging neutron stars or neutron stars–black hole collisions.
    • Long GRBs: Lasting 2–1000 seconds, arising from supernova collapses of massive stars (collapsars).
  • Energy Output: A single GRB can release as much energy in seconds as the Sun emits over its entire lifetime (~10⁵¹–10⁵⁴ ergs).
  • Afterglow: Follows the main burst in X-ray, optical, and radio wavelengths, allowing astronomers to study host galaxies and distances.

Hypothesis about Black Hole ‘Morsels’:

  • Study Context: Research proposes the existence of “black hole morsels”, tiny remnants formed during black hole mergers.
  • Formation Mechanism: During merger, spacetime “pinches off” into ultra-dense pockets, creating micro-black holes or morsels that may later evaporate.
  • Emissions: These morsels are predicted to release gamma rays and high-energy particles via Hawking radiation, providing a possible observational signature of quantum gravity.
  • Scientific Goal: The hypothesis aims to bridge general relativity and quantum mechanics, offering a natural test case for quantum spacetime dynamics.

What are Black Hole Morsels?

  • Overview: Hypothetical micro–black holes formed as fragments during black hole mergers under extreme gravitational stress.
  • Origin: Result from pinched-off regions of spacetime during coalescence of two black holes.
  • Mass & Size: Much smaller than parent black holes, roughly asteroid-scale mass but with extreme density.
  • Temperature & Radiation: Extremely hot, emitting intense Hawking radiation– photons, neutrinos, and high-energy particles.
  • Lifetime: Short-lived — ranging from milliseconds to years, depending on initial mass.
  • Detectability: Expected to produce isotropic gamma-ray bursts, unlike directional jets of typical GRBs.
  • Observation Instruments: Potential detection via HESS (Namibia), HAWC (Mexico), LHAASO (China), and Fermi Space Telescope (USA).

Scientific Significance:

  • Quantum Gravity Evidence: Detection would confirm that gravity behaves quantum mechanically at microscopic scales.
  • Spacetime Structure: Provides direct insight into the quantum texture of spacetime near black hole singularities.
  • Cosmic Accelerator Analogy: Morsels could probe energy scales far beyond the LHC, acting as natural high-energy laboratories.
  • Current Status: None observed yet, but existing gamma-ray data are being analysed to set upper mass limits and refine the model.
[UPSC 2019] Recently, scientists observed the merger of giant ‘Blackholes’ billions of light-years away from the Earth. What is the significance of this observation?

Options: (a) Higgs boson particles were detected.

(b) Gravitational waves were detected.*

(c) Possibility of inter-galactic space travel through ‘wormhole’ was confirmed.

(d) It enabled the scientists to understand ‘singularity’.

 

Get an IAS/IPS ranker as your 1: 1 personal mentor for UPSC 2024

Attend Now

Subscribe
Notify of
0 Comments
Oldest
Newest Most Voted
Inline Feedbacks
View all comments

JOIN THE COMMUNITY

Join us across Social Media platforms.