Graduate Action for quintessence

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SUMMARY

Kislev developed a black hole metric in the quintessence field by analyzing the energy-momentum tensor with the condition $T^t_t=T^r_r$. This approach raises the question of whether there exists an action for the quintessence field that produces this specific energy-momentum tensor upon variation with respect to the metric tensor $g^{\mu \nu}$. The discussion emphasizes the need for a specific reference to Kislev's work for further examination of these concepts.

PREREQUISITES
  • Understanding of quintessence in cosmology
  • Familiarity with energy-momentum tensors
  • Knowledge of metric tensors in general relativity
  • Experience with variational principles in theoretical physics
NEXT STEPS
  • Research the concept of quintessence in cosmological models
  • Examine the derivation of energy-momentum tensors in general relativity
  • Study variational principles and their applications in field theories
  • Locate and analyze Kislev's referenced paper for detailed methodologies
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The discussion is beneficial for theoretical physicists, cosmologists, and researchers interested in advanced topics related to quintessence and black hole metrics.

djymndl07
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Kislev developed black hole metric in quintessence field by considering $T^t_t=T^r_r$ for energy momentum tesor corresponding to quintessence. Is there any action for the quintessence fild that gives such energy momentum tensor after varying with respect to $g^{\mu \nu}$?
 
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djymndl07 said:
Kislev developed black hole metric in quintessence field...
Can you please cite the specific Kislev reference so we can take a look?
 
renormalize said:
Can you please cite the specific Kislev reference so we can take a look?
Sure. Please see This paper for reference.
 
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