Flat spacetime + gravitons = Curved spacetime?

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Discussion Overview

The discussion centers on the relationship between flat spacetime and the emergence of curvature through the presence of gravitons, exploring theoretical implications and interpretations within the context of general relativity and string theory. Participants reference historical claims and literature, including works by Steve Carlip and Misner, Thorne, & Wheeler.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions whether flat spacetime plus gravitons necessarily leads to curved spacetime, referencing Steve Carlip's assertion about the need for a massless spin-two interaction.
  • Another participant cites Bill Hobba's claim that the underlying geometry of spacetime in string theory is not known and suggests that curvature may emerge rather than being inherent.
  • A later reply discusses the implications of coupling the spin-2 field to the total stress-tensor, suggesting that the original flat background spacetime becomes unobservable, leading to an effective Riemannian space.
  • One participant mentions that if spacetime can be covered by harmonic coordinates, then curvature can be equivalent to a spin-2 field on flat spacetime.
  • Another participant proposes that there should be testable predictions regarding phenomena like re-radiation from objects falling into black holes, questioning the seriousness with which these theories are treated by their proponents.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between flat spacetime and curvature, with no consensus reached on whether gravitons inherently lead to curvature or if it is merely an emergent property. The discussion remains unresolved regarding the implications of these theories and their testability.

Contextual Notes

Participants reference various theoretical frameworks and historical claims, indicating that assumptions about the nature of spacetime and graviton interactions may not be universally accepted. The discussion highlights the complexity and nuance of the topic, with unresolved mathematical and conceptual steps.

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Hi, does flat spacetime + gravitons automatically lead to curved spacetime?

In an old 2002 google thread sci.physics.research which is moderated:

http://groups.google.com/group/sci....Einstein+Field+Equations+and+Flat+Space+Time#

Steve Carlip seemed to agree when he said:

"There's a bit more to it. You also need, at least, a massless spin two interaction that couples universally. While this doesn't involve general covariance in an obvious way, a massless spin two field has a gauge invariance that's ``as big'' as diffeomorphism invariance (i.e., that's parametrized by a vector field), and the universality of the coupling rules out any noninvariant ``background.''

Steve Carlip"

Bill Hobba who is now a member of Physicsforums wrote this at sci.physics. (need comment how true it is).

Someone asked (in 2002) at sci.physics: "But in string theory, spacetime still has curvature."

Bill Hobba replied all the following:

"No it doesn't. It emerges as a limit - but the underlying geometry of space-time - if it has one - is not known."

"As Steve Carlip once explained, it is experimentally impossible to tell a theory formulated in flat space-time that makes rulers and clocks behave as if it was curved from a curved one, so the question is basically meaningless at our current level of knowledge."

"Up to about the plank scale the assumption it is flat is fine, with gravitons making it behave like it had curvature or actually giving it curvature (we can't determine which) works quite well. "

True? If yes, how much is it supported in String Theory? If not, why?
 
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Looking at this matter further. I found out it was not even original claim by Steve Carlip but direct from Misner, Thorne, & Wheeler's book "Gravitation". I saw the following in Physicsforums:

https://www.physicsforums.com/showthread.php?t=278874

"Is spacetime really curved? Embedded somewhere?

Message #4:

"There's a fascinating analysis due to Deser ["Self-interaction and
gauge invariance", General Relativity & Gravitation 1 (1970), 9-18;
see also his later paper "Gravity from self-interaction in a curved
background", Classical and Quantum Gravity 4 (1997), L99-L105],
summarized in part 5 of box 17.2 of Misner, Thorne, & Wheeler's book.

Quoting from that latter summary:

"The Einstein equations may be derived nongeometrically by
noting that the free, massless, spin-2 field equations
[[for a field $\phi$]]
[[...]]
whose source is the matter stress-tensor $T_{\mu\nu}$, must
actually be coupled to the \emph{total} stress-tensor,
including that of the $\phi$-field itself.
[[...]]
Consistency has therefore led us to universal coupling, which
implies the equivalence principle. It is at this point that
the geometric interpretation of general relativity arises,
since \emph{all} matter now moves in an effective Riemann space
of metric $\mathcal{g}^{\mu\nu} = \eta^{\mu\nu} + h^{\mu\nu}$.
... [The] initial flat `background' space is no longer observable."

In other words, if you start off with a spin-2 field which lives on a
flat "background" spacetime, and say that its source term should include
the field energy, you wind up with the original "background" spacetime
being *unobservable in principle*, i.e. no possible observation can
detect it. Rather, *all* observations will now detect the effective
Riemannian space (which is what the usual geometric interpretation of
general relativity posits from the beginning)."

Comment?
 
Check out the full arguments here in Misner, Thorne, Wheeler "Gravitation":

http://www.scribd.com/doc/81449908/Flat-spacetime-Gravitons

See the starting lines at :
5. Einstein's geometrodynamics viewed as the standard field theory for a field of spin 2 in an "unobservable flat spacetime" background

(body of arguments)

ending at
"
...[The] initial flat 'background' space is no longer observable." In other words, this approach to Einstein's field equation can be summarized as "curvature without curvature" or - equally well - as "flat spacetime without flat spacetime"!"

What do you think?
 
Yes. If spacetime can be covered by harmonic coordinates, then spacetime curvature is equivalent to a spin 2 field on a flat spacetime.

An introduction can be found in http://arxiv.org/abs/astro-ph/0006423
 
I think there should actually be some testable predictions if these theories are really taken seriously, about re-radiation from things falling into black holes. But it seems that the authors of these sort of theories don't really takes them seriously enough to calculate this in detail.
 

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