Event

Feb 12, 2018
Is the Standard Theory of Semiclassical Einstein Gravity Viable?

The self-consistency and empirical viability of standard semiclassical Einstein gravity (SSEG), viewed either as a fundamental theory or a mean-field approximation to some theory of quantum gravity, will be discussed. It will be shown that

  1. SSEG, when viewed as a fundamental theory, is either not self-consistent or empirically ruled out (depending on how the matter side of the theory is interpreted); and
  2. SSEG, when viewed as a mean-field approximation to a quantum gravity theory, has a domain of applicability that's much more limited than is widely assumed; and
  3. the assumptions underlying the mean-field approximations in (2) are either physically inconsistent, ad hoc, or unrealistic.

It will then be shown that the aforementioned problems with the SSEG invalidate well-known applications of SSEG to astrophysics and cosmology; notably, Hawking's 1975 argument for black hole evaporation (and refinements thereof), the cosmological constant problem, arguments for the stability / instability of traversable wormholes and warp drive spacetimes, and cosmological perturbations in inflation. Historical context will be given throughout, including reference to the work of Moller and Rosenfeld in the 1960s, the subsequent work of the 70s and 80s on foundational issues in SSEG and renormalization/regularization techniques to make SSEG mathematically well-defined, the work of the 90's and 2000's on "stochastic gravity" (an extension of the of the SSEG), and work in the 2000s and 2010s connecting SSEG to "gravitational decoherence" proposals.  

 

Organizer(s)
Address

Harnackstraße 5, Berlin 14195, Germany

Room
Villa, Room V005/Seminar Room
Contact and Registration

All welcome, no registration necessary. For further information email officeblum@mpiwg-berlin.mpg.de.

 

About This Series

The seminar of the Research Group “Historical Epistemology of the Final Theory Program” runs once a month, usually on a Monday at 14:30 in the seminar room of the Villa (Harnackstraße 5). The talks deal primarily with the history, philosophy, and foundations of modern (post-WWII) physics or with wider epistemological questions related to the work of the group. There are no pre-circulated papers.

 

2018-02-12T14:30:00SAVE IN I-CAL 2018-02-12 14:30:00 2018-02-12 16:00:00 Is the Standard Theory of Semiclassical Einstein Gravity Viable? The self-consistency and empirical viability of standard semiclassical Einstein gravity (SSEG), viewed either as a fundamental theory or a mean-field approximation to some theory of quantum gravity, will be discussed. It will be shown that SSEG, when viewed as a fundamental theory, is either not self-consistent or empirically ruled out (depending on how the matter side of the theory is interpreted); and SSEG, when viewed as a mean-field approximation to a quantum gravity theory, has a domain of applicability that's much more limited than is widely assumed; and the assumptions underlying the mean-field approximations in (2) are either physically inconsistent, ad hoc, or unrealistic. It will then be shown that the aforementioned problems with the SSEG invalidate well-known applications of SSEG to astrophysics and cosmology; notably, Hawking's 1975 argument for black hole evaporation (and refinements thereof), the cosmological constant problem, arguments for the stability / instability of traversable wormholes and warp drive spacetimes, and cosmological perturbations in inflation. Historical context will be given throughout, including reference to the work of Moller and Rosenfeld in the 1960s, the subsequent work of the 70s and 80s on foundational issues in SSEG and renormalization/regularization techniques to make SSEG mathematically well-defined, the work of the 90's and 2000's on "stochastic gravity" (an extension of the of the SSEG), and work in the 2000s and 2010s connecting SSEG to "gravitational decoherence" proposals.     MPIWG Alexander Blum admin@example.com Europe/Berlin public