Einstein Hilbert action

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SUMMARY

The discussion centers on the relationship between the Lagrangian density term in the Einstein-Hilbert action and the Ricci scalar in the context of gravitational fields. It references Carroll's notes, highlighting that the Ricci scalar is the simplest scalar containing up to second-order derivatives of the metric. The conversation also touches on modified gravity theories, which utilize a general function f(R), emphasizing that to recover General Relativity (GR), f(R) must approximate R in leading order.

PREREQUISITES
  • Understanding of the Einstein-Hilbert action
  • Familiarity with Ricci scalar and its significance in general relativity
  • Knowledge of Lagrangian density in physics
  • Concepts of modified gravity theories and their implications
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  • Research the derivation of the Einstein-Hilbert action in detail
  • Study the properties and applications of the Ricci scalar in general relativity
  • Explore various modified gravity theories and their mathematical formulations
  • Examine the implications of f(R) theories on cosmology and astrophysics
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Physicists, cosmologists, and students of general relativity seeking to deepen their understanding of gravitational theories and the mathematical foundations of the Einstein-Hilbert action.

Das apashanka
My question is why is the lagrangian density term in the action is equal to ricci scaler for gravitational field
 
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See e.g. Carroll's notes: it's the simplest scalar which contains up to second order derivatives of the metric. But maybe 'why' is the wrong question. We don't know 'why'. But it works.
 
It might be mentioned in this context that many theories of modified gravity instead put a general function ##f(R)##. Of course, to recover GR you need ##f(R) \simeq R## to leading approximation.
 

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