Physics:Hawking energy

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Short description: One of the possible definitions of mass in general relativity

The Hawking energy or Hawking mass is one of the possible definitions of mass in general relativity. It is a measure of the bending of ingoing and outgoing rays of light that are orthogonal to a 2-sphere surrounding the region of space whose mass is to be defined.

Definition

Let (3,gab) be a 3-dimensional sub-manifold of a relativistic spacetime, and let Σ3 be a closed 2-surface. Then the Hawking mass mH(Σ) of Σ is defined[1] to be

mH(Σ):=AreaΣ16π(1116πΣH2da),

where H is the mean curvature of Σ.

Properties

In the Schwarzschild metric, the Hawking mass of any sphere Sr about the central mass is equal to the value m of the central mass.

A result of Geroch[2] implies that Hawking mass satisfies an important monotonicity condition. Namely, if 3 has nonnegative scalar curvature, then the Hawking mass of Σ is non-decreasing as the surface Σ flows outward at a speed equal to the inverse of the mean curvature. In particular, if Σt is a family of connected surfaces evolving according to

dxdt=1Hν(x),

where H is the mean curvature of Σt and ν is the unit vector opposite of the mean curvature direction, then

ddtmH(Σt)0.

Said otherwise, Hawking mass is increasing for the inverse mean curvature flow.[3]

Hawking mass is not necessarily positive. However, it is asymptotic to the ADM[4] or the Bondi mass, depending on whether the surface is asymptotic to spatial infinity or null infinity.[5]

See also

References

  1. Page 21 of Schoen, Richard, 2005, "Mean Curvature in Riemannian Geometry and General Relativity," in Global Theory of Minimal Surfaces: Proceedings of the Clay Mathematics Institute 2001 Summer School, David Hoffman (Ed.), pp. 113–136.
  2. Geroch, Robert (1973). "Energy Extraction". Annals of the New York Academy of Sciences 224: 108–117. doi:10.1111/j.1749-6632.1973.tb41445.x. Bibcode1973NYASA.224..108G. 
  3. Lemma 9.6 of Schoen (2005).
  4. Section 4 of Yuguang Shi, Guofang Wang and Jie Wu (2008), "On the behavior of quasi-local mass at the infinity along nearly round surfaces".
  5. Section 2 of Finster, Felix; Smoller, Joel; Yau, Shing-Tung (2000). "Some recent progress in classical general relativity". Journal of Mathematical Physics 41 (6): 3943–3963. doi:10.1063/1.533332. Bibcode2000JMP....41.3943F. 

Further reading