Vacuum energy density from the form factor bootstrap
Abstract The form-factor bootstrap is incomplete until one normalizes the zero-particle form factor. For the stress energy tensor we describe how to obtain the vacuum energy density ρ vac, defined as 〈0|T μν |0〉 = ρ vac g μν , from the form-factor bootstrap. Even for integrable QFT’s in D=2 spacetim...
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2024-12-01
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| Series: | Journal of High Energy Physics |
| Subjects: | |
| Online Access: | https://doi.org/10.1007/JHEP12(2024)110 |
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| Summary: | Abstract The form-factor bootstrap is incomplete until one normalizes the zero-particle form factor. For the stress energy tensor we describe how to obtain the vacuum energy density ρ vac, defined as 〈0|T μν |0〉 = ρ vac g μν , from the form-factor bootstrap. Even for integrable QFT’s in D=2 spacetime dimensions, this prescription is new, although it reproduces previously known results obtained in a different and more difficult thermodynamic Bethe ansatz computation. We propose a version of this prescription in D=4 dimensions. For these even dimensions, the vacuum energy density has the universal form ρ vac ∝ m D / g $$ {\rho}_{\textrm{vac}}\propto {m}^D/\mathfrak{g} $$ where g $$ \mathfrak{g} $$ is a dimensionless interaction coupling constant which can be determined from the high energy behavior of the S-matrix. In the limit g → 0 $$ \mathfrak{g}\to 0 $$ , ρ vac diverges due to well understood UV divergences in free quantum field theories. If we assume the observed Cosmological Constant originates from the vacuum energy density ρ vac computed as proposed here, then this suggests there must exist a particle which does not obtain its mass from spontaneous symmetry breaking in the electro-weak sector, which we designate as the “zeron”. A strong candidate for the zeron is a massive Majorana neutrino. |
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| ISSN: | 1029-8479 |