String theory deviations from GR in strong field regime

Click For Summary
String theory is characterized as a scalar-tensor theory of gravity with higher order corrections. Recent discoveries of gravitational waves from black hole mergers align with General Relativity (GR) in the strong field regime, raising questions about potential deviations from GR predicted by string theory. Current understanding suggests that string theory does not contribute to gravitational wave generation, which is a classical aspect of GR. Scalar-tensor theories, including string theory, do not produce different outputs for gravitational waves compared to GR. Consequently, the strong field regime does not currently provide conclusive evidence for or against string theory as a viable theory of quantum gravity.
kodama
Messages
1,083
Reaction score
144
string theory is a scalar-tensor theory of gravity, with higher order corrections. in light of the result discovery of gravitational waves of 2 black holes merging, matching GR in the strong field regime, how much deviation should strong theory differ from GR in the strong field regime and can LIGO detect them?

if results continue to match GR in the strong field regime and not match up with string theory, how would this affect string as a theory of QG
 
Physics news on Phys.org
The usual process to generate gravitational waves is part of classical GRT. Currently there is no contribution of quantum gravity to this part. Therefore sring theory is also not able to produce any contribution to this topic. As far as I know scalar-tensor theories do not produce a different output for gravitational waves then GRT. The higher order corrections (in a sense of an effective theory) have more the effect to prevent the singularity (see also http://arxiv.org/abs/1512.08346).
So currently, the strong field regime cannot decide about the trueness of string theory.
 
  • Like
Likes kodama
"Supernovae evidence for foundational change to cosmological models" https://arxiv.org/pdf/2412.15143 The paper claims: We compare the standard homogeneous cosmological model, i.e., spatially flat ΛCDM, and the timescape cosmology which invokes backreaction of inhomogeneities. Timescape, while statistically homogeneous and isotropic, departs from average Friedmann-Lemaître-Robertson-Walker evolution, and replaces dark energy by kinetic gravitational energy and its gradients, in explaining...

Similar threads

  • · Replies 15 ·
Replies
15
Views
5K
  • · Replies 60 ·
3
Replies
60
Views
7K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 6 ·
Replies
6
Views
6K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 105 ·
4
Replies
105
Views
15K
  • · Replies 2 ·
Replies
2
Views
5K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 0 ·
Replies
0
Views
4K