Inertial mass of an elementary particle from the holographic scenario
Various attempts have been made to fully explain the mechanism by which a body has inertial mass. Recently it has been proposed that this mechanism is as follows: when an object accelerates in one direction a dynamical Rindler event horizon forms in the opposite direction, suppressing Unruh radiatio...
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| Tipo de recurso: | artículo |
| Estado: | Versión aceptada para publicación |
| Fecha de publicación: | 2017 |
| País: | España |
| Institución: | Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
| Repositorio: | Recercat. Dipósit de la Recerca de Catalunya |
| OAI Identifier: | oai:recercat.cat:10459.1/62944 |
| Acceso en línea: | https://doi.org/10.1142/S0217751X17500439 http://hdl.handle.net/10459.1/62944 |
| Access Level: | acceso abierto |
| Palabra clave: | Inertial mass Unruh radiation Holographic scenario Dark matter Dark energy Cosmology |
| Sumario: | Various attempts have been made to fully explain the mechanism by which a body has inertial mass. Recently it has been proposed that this mechanism is as follows: when an object accelerates in one direction a dynamical Rindler event horizon forms in the opposite direction, suppressing Unruh radiation on that side by a Rindler-scale Casimir effect whereas the radiation in the other side is only slightly reduce by a Hubble-scale Casimir effect. This produces a net Unruh radiation pressure force that always opposes the acceleration, just like inertia, although the masses predicted are twice those expected, see \cite{Mc6}. In a later work an error was corrected so that its prediction improves to within 26\% of the Planck mass, see \cite{GM}. In this paper the expression of the inertial mass of a elementary particle is derived from the holographic scenario giving the exact value of the mass of a Planck particle when it is applied to a Planck particle. |
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