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Vacuum energy and relativistic invariance

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arxiv hep-th/0204048 v2 pith:GAKWUCCW submitted 2002-04-04 hep-th astro-phgr-qchep-ph

classification hep-thastro-phgr-qchep-ph
keywords consequenceenergiesenergyfieldsfreeinvariancerelativisticvacuum
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abstract

It is argued that the zero-point energies of free quantum fields diverge at most quadratically and not quartically, as is generally believed. This is a consequence of the relativistic invariance which requires that the energy density of the vacuum $\rho$ and its pressure $p$ satisfy $\rho=-p$. The usually obtained quartic divergence is an artifact of the use of a noninvariant regularization which violates this relation. One consequence of our results is that the zero-point energies of free massless fields vanish. Implications for the cosmological constant problem are briefly discussed.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum

    gr-qc 2026-01 conditional novelty 6.0 of 10

    The vacuum energy of quantum fields, computed exactly in de Sitter spacetime and then allowed to decay into radiation, can drive H^4-powered inflation and leave a slowly running dark energy δρ_vac ~ m_Pl^2 H^2, unifyi...

  2. Logarithmically Divergent Vacuum Energy in Effective Field Theory

    hep-th 2025-07 reject novelty 4.0 of 10

    The paper reports that random boson and fermion spectra forced to respect a Lorentz-invariant vacuum produce a vacuum energy distribution whose width grows only logarithmically with the ultraviolet cutoff.

  3. Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy

    gr-qc 2026-06 unverdicted novelty 3.0 of 10

    The running vacuum model derives dynamical vacuum energy from QFT in curved spacetime, using H^4 terms for inflation and H^2 terms for dark energy while G evolves logarithmically.

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