Derivation of Einstein Field Equations

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SUMMARY

The discussion focuses on the derivation of the Einstein Field Equations as presented in Sean M. Carroll's "Spacetime and Geometry: An Introduction to General Relativity." The equation R_{\mu\nu}-\frac{1}{2} Rg_{\mu\nu}=\kappa T_{\mu\nu} is analyzed, particularly the contraction leading to R=-\kappa T. A common misunderstanding arises from the treatment of the metric tensor g_{\mu\nu}, where participants clarify that g^\mu_\mu equals 4, not 1, which resolves the confusion. The importance of consulting the book's errata is emphasized to avoid misinterpretations due to potential typos.

PREREQUISITES
  • Understanding of Ricci tensor (R_{\mu\nu}) and stress-energy tensor (T_{\mu\nu})
  • Familiarity with the metric tensor (g_{\mu\nu}) and its properties
  • Basic knowledge of tensor contraction in differential geometry
  • Awareness of general relativity concepts as discussed in Carroll's work
NEXT STEPS
  • Review the derivation of the Einstein Field Equations in "Spacetime and Geometry" by Sean M. Carroll
  • Study the properties of the metric tensor and its role in general relativity
  • Explore the implications of the Einstein Field Equations on cosmology and astrophysics
  • Check the errata page for "Spacetime and Geometry" for any corrections or clarifications
USEFUL FOR

Students of general relativity, physicists, and anyone studying the mathematical foundations of the Einstein Field Equations will benefit from this discussion.

tensor33
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I'm reading Spacetime and Geometry: An Introduction to General Relativity by Sean M. Carrol and in the chapter on gravitation, he derives the Einstein Field Equations. Here is the part I don't get. He starts with the equation R_{\mu\nu}-\frac{1}{2} Rg_{\mu\nu}=\kappa T_{\mu\nu} Wher R_{\mu\nu} is the Ricci tensor, \kappa is some constant, and T_{\mu\nu} is the stress-energy tensor. Then he sates that by contracting both sides it becomes,R=-\kappa T where R=R_{\mu\nu}g^{\mu\nu} and T=T_{\mu\nu}g^{\mu\nu}. I don't see how he came to this answer. When I tried to work it out myself I got R=2\kappa T This obviously isn't the right answer, and I can't see what I'm missing. I'm drawing a blank here.
 
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g_{\mu\nu}g^{\mu\nu}=4
 
g^{\mu \nu }R_{\mu \nu } - \frac{1}{2}Rg^{\mu \nu }g_{\mu \nu } = R - \frac{1}{2}R\delta ^{\mu }_{\mu } = R - 2R = - R = \kappa T
EDIT: robphy beat me to it =D
 
I made the same mistake as you the first time I did it. Although g^\mu_\nu has diagonal *elements* that all equal 1, that doesn't mean you can replace it with 1 when you contract. It has four diagonal elements, so g^\mu_\mu=4.
 
Oh! It all makes sense now! I wish Carroll would've been a little more explicit in that step, it would've saved me a lot of confusion. Oh well. At least I get it now, thanks to all those who replied.
 
tensor33 said:
Oh! It all makes sense now! I wish Carroll would've been a little more explicit in that step, it would've saved me a lot of confusion. Oh well. At least I get it now, thanks to all those who replied.
In the future however, make sure you check his errata page because the book does have a ton of errata and in the event that he did make a typo, you don't want to rip your hair out when your result is correct but the thing in the book says something else.
 
WannabeNewton said:
In the future however, make sure you check his errata page because the book does have a ton of errata and in the event that he did make a typo, you don't want to rip your hair out when your result is correct but the thing in the book says something else.

Thanks I'll make sure to keep that in mind.
 

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