Matter non-conservation in the universe and dynamical dark energy
In an expanding universe, the vacuum energy density ρ Λ is expected to be a dynamical quantity. In quantum field theory in curved spacetime, ρ Λ should exhibit a slow evolution, determined by the expansion rate of the universe H. Recent measurements on the time variation of the fine-structure consta...
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Main Authors: | Fritzsch, Harald., Solà, Joan. |
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Other Authors: | Institute of Advanced Studies |
Format: | Article |
Language: | English |
Published: |
2013
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Online Access: | https://hdl.handle.net/10356/96888 http://hdl.handle.net/10220/13064 |
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Institution: | Nanyang Technological University |
Language: | English |
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