MeV Dark Energy Emission from a De Sitter Universe
The evolution of a de Sitter Universe is the basis for both the accelerated Universe and the late-stationary Universe. So, how do we differentiate between both universes? In this paper, we state that it is not possible to design an experiment using luminous or angular distances to distinguish betwee...
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| Format: | Article |
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MDPI AG
2023-12-01
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| Series: | Universe |
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| Online Access: | https://www.mdpi.com/2218-1997/9/12/513 |
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| author | Yasmín B. Alcántara-Pérez Miguel. A. García-Aspeitia Humberto Martínez-Huerta Alberto Hernández-Almada |
| author_facet | Yasmín B. Alcántara-Pérez Miguel. A. García-Aspeitia Humberto Martínez-Huerta Alberto Hernández-Almada |
| author_sort | Yasmín B. Alcántara-Pérez |
| collection | DOAJ |
| description | The evolution of a de Sitter Universe is the basis for both the accelerated Universe and the late-stationary Universe. So, how do we differentiate between both universes? In this paper, we state that it is not possible to design an experiment using luminous or angular distances to distinguish between the two cases because they are the same during the de Sitter phase. However, this equivalence allows us prediction of the signal of <i>a constant dark energy emission</i> with a signal peak around 29.5 MeV, in which, according to our astrophysical test of survival probability, the radiation must be <i>non-standard photons</i>. Remarkably, experiments by EGRET and COMPTEL have observed an excess of gamma photons in this predicted region, coming from a possible decay process of dark energy emission, which may constitute the smoking gun of a late-stationary Universe with the continuous creation of non-standard radiation, an alternative approach to understanding the current stages of the Universe’s evolution. |
| first_indexed | 2024-03-08T20:19:24Z |
| format | Article |
| id | doaj.art-b4e8fb2bacd74bb5970e2d7578b041c8 |
| institution | Directory Open Access Journal |
| issn | 2218-1997 |
| language | English |
| last_indexed | 2024-03-08T20:19:24Z |
| publishDate | 2023-12-01 |
| publisher | MDPI AG |
| record_format | Article |
| series | Universe |
| spelling | doaj.art-b4e8fb2bacd74bb5970e2d7578b041c82023-12-22T14:46:37ZengMDPI AGUniverse2218-19972023-12-0191251310.3390/universe9120513MeV Dark Energy Emission from a De Sitter UniverseYasmín B. Alcántara-Pérez0Miguel. A. García-Aspeitia1Humberto Martínez-Huerta2Alberto Hernández-Almada3Departamento de Física, DCI, Campus León, Universidad de Guanajuato, León 37150, Guanajuato, MexicoDepartamento de Física y Matemáticas, Universidad Iberoamericana, Prolongación Paseo de la Reforma 880, Mexico 01219, MexicoDepartamento de Física y Matemáticas, Universidad de Monterrey, Av. Morones Prieto 4500, San Pedro Garza García 66238, Nuevo León, MexicoFacultad de Ingeniería, Universidad Autónoma de Querétaro, Centro Universitario Cerro de las Campanas, Santiago de Querétaro 76010, MexicoThe evolution of a de Sitter Universe is the basis for both the accelerated Universe and the late-stationary Universe. So, how do we differentiate between both universes? In this paper, we state that it is not possible to design an experiment using luminous or angular distances to distinguish between the two cases because they are the same during the de Sitter phase. However, this equivalence allows us prediction of the signal of <i>a constant dark energy emission</i> with a signal peak around 29.5 MeV, in which, according to our astrophysical test of survival probability, the radiation must be <i>non-standard photons</i>. Remarkably, experiments by EGRET and COMPTEL have observed an excess of gamma photons in this predicted region, coming from a possible decay process of dark energy emission, which may constitute the smoking gun of a late-stationary Universe with the continuous creation of non-standard radiation, an alternative approach to understanding the current stages of the Universe’s evolution.https://www.mdpi.com/2218-1997/9/12/513cosmological constantcosmology |
| spellingShingle | Yasmín B. Alcántara-Pérez Miguel. A. García-Aspeitia Humberto Martínez-Huerta Alberto Hernández-Almada MeV Dark Energy Emission from a De Sitter Universe Universe cosmological constant cosmology |
| title | MeV Dark Energy Emission from a De Sitter Universe |
| title_full | MeV Dark Energy Emission from a De Sitter Universe |
| title_fullStr | MeV Dark Energy Emission from a De Sitter Universe |
| title_full_unstemmed | MeV Dark Energy Emission from a De Sitter Universe |
| title_short | MeV Dark Energy Emission from a De Sitter Universe |
| title_sort | mev dark energy emission from a de sitter universe |
| topic | cosmological constant cosmology |
| url | https://www.mdpi.com/2218-1997/9/12/513 |
| work_keys_str_mv | AT yasminbalcantaraperez mevdarkenergyemissionfromadesitteruniverse AT miguelagarciaaspeitia mevdarkenergyemissionfromadesitteruniverse AT humbertomartinezhuerta mevdarkenergyemissionfromadesitteruniverse AT albertohernandezalmada mevdarkenergyemissionfromadesitteruniverse |