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  2. 4 The Einstein Equations‣ General Relativity by David Tong

    www.damtp.cam.ac.uk/user/tong/gr/grhtml/S4.html
    16 Oct 2021: Before we proceed, a small comment. We happily discarded the boundary term in (4.149), a standard practice whenever we invoke the variational principle. ... In such circumstances, one can be more careful by invoking the so-called Gibbons-Hawking boundary
  3. 10 May 2024: The final term vanishes. because we have fixed the end points of the path. ... term gives us a potential V (x) = qϕ(x) of the kind we wanted.
  4. 4. The Einstein Equations It is now time to ...

    www.damtp.cam.ac.uk/user/tong/gr/four.pdf
    25 Feb 2021: in Section 6. Before we proceed, a small comment. We happily discarded the boundary term in. ... Gibbons-Hawking boundary term. – 143 –. 4.1.1 An Aside on Dimensional Analysis.
  5. 4 Sep 2014: There is also the standard Gibbons-. Hawking boundary term which we have not written explicitly. ... as an F-term [17, 18] (using the so-called “chiral projection operator”).
  6. Field Theory in Cosmology (Part III) Enrico Pajer Contents ...

    www.damtp.cam.ac.uk/user/ep551/field_theory_in_Cosmology.pdf
    15 Apr 2021: field with. the wrong-sing kinetic term that can be created at will by decreasing the energy of the. ... S =. g[. 1. 2M2PlR P(X,φ). ], (1.55). where X represents the standard canonical kinetic term,.

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