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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Rami Ahmad El-Nabulsi | en_US |
dc.date.accessioned | 2022-10-16T07:29:52Z | - |
dc.date.available | 2022-10-16T07:29:52Z | - |
dc.date.issued | 2021-01-01 | en_US |
dc.identifier.issn | 00084204 | en_US |
dc.identifier.other | 2-s2.0-85104272573 | en_US |
dc.identifier.other | 10.1139/cjp-2020-0193 | en_US |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85104272573&origin=inward | en_US |
dc.identifier.uri | http://cmuir.cmu.ac.th/jspui/handle/6653943832/77389 | - |
dc.description.abstract | In this communication, a conformal coupling gravity is discussed in the presence of a complex Coleman-Weinberg potential, which is generated from the contributions from first-, second-, and all higher-order loops. A relation between the cosmological constant, the Hubble mass, and the Higgs vacuum energy is obtained in particular when Weinberg-Landau gauge is used. Moreover, it was observed that the removal of the logarithmic mass boosts the scalar mass from Hubble mass of order 10-33 eV to 2.47 10-3 eV, which is comparable to the mass of non-baryonic cold dark matter or axion based on recent observations and which constitutes about 84% of all matter in the Universe. | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Cosmological constant, planck mass, hubble mass, and axion: A relation through higher-order loops coleman-weinberg potential with weinberg-landau gauge | en_US |
dc.type | Journal | en_US |
article.title.sourcetitle | Canadian Journal of Physics | en_US |
article.volume | 99 | en_US |
article.stream.affiliations | Shenzhen Technology University | en_US |
article.stream.affiliations | Chiang Mai University | en_US |
article.stream.affiliations | Athens Institute for Education and Research | en_US |
Appears in Collections: | CMUL: Journal Articles |
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