Non-local partner to the cosmological constant

preprint2022arXivOpen access

Abstract

I show that quantum corrections due to a massive particle generates a non-local term in the gravitational effective action which is of zeroth order in the derivative expansion, much like the cosmological constant. It carries a fixed coefficient which is very much larger than the cosmological constant, and which cannot be fine-tuned. The interaction is active at scales above the particle's mass. This is of the form m4(1□R)x"<x∣log⁡(□+m2)∣y>"(1□R)ym^4 (\frac1{\Box}R)_x "<x|\log (\Box +m^2 )|y >" (\frac1{\Box}R)_y, and I discuss the meaning of "<x∣log⁡(□+m2)∣y>" "<x|\log (\Box +m^2) |y >" and other aspects of its interpretation.

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