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Brustein, Ram

Brustein, Ram
54/313 54/315
Research type
Research topics

Black Holes; Cosmology; Gravitation; String theory

Researcher identification
Google Scholar, ResearcherID, ORCID


Research group

  1. MSc student, Lilian Saiegh
  2. PhD student, Shani Avitan
  3. PhD student, Hagar Meir
  4. PhD student, Tom Shindelman
  5. PhD student, Tamar Simhon

Past graduate students *

  1. Chana Hausmann, MSc (2023)
  2. Yoav Zigdon, PhD (2023)
  3. Yotam Sherf, PhD (2023)
  4. Ira Wolfson, PhD (2019)
  5. Yoav Zigdon, MSc (2019)
  6. Itay Raveh, MSc (2019)
  7. Ira Wolfson, MSc (2018)
  8. Yotam Sherf, MSc (2018)
  9. Daniel Levy, PhD (2018)
  10. Yael Raveh, MSc (2018)
  11. Amos Yarom, PhD (2018)

Past undergraduate students *

  1. Lipaz Aspir (2021)
* Past students / postdocs data might be incomplete

Research highlights

Quantum gravity & quantum black holes

Quantum black hole swallows matter and evaporates quantum mechanically

Are Einstein's equations and general relativity compatible with quantum mechanics? In spite of intense efforts over the last 40 years by some of the best physicists we still do not know the answer .

I study the properties of black holes and other space-times with horizons to probe the laws of quantum gravity. Based on our recent research, our proposed answer is: Yes. The apparent incompatibilities between general relativity and quantum mechanics originate from the extreme approximation of treating spacetime as a strictly classical geometric object.


A new class of cosmic inflation models

The early universe is used as a theoretical laboratory for studying fundamental physics, the laws of gravity and quantum mechanical aspects of matter under extreme conditions.

We study models of cosmic inflation in the early universe and dark energy in the late universe and their possible realizations in quantum field theory and string theory models.

Our recent research focuses on models of high-scale inflation which produce an observable signal of gravitational waves in the cosmic microwave background.

Additional research highlights