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| Format: | Preprint |
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2024
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| Online Access: | https://arxiv.org/abs/2410.02036 |
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| _version_ | 1866909685463908352 |
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| author | Marmet, L. |
| author_facet | Marmet, L. |
| contents | The gradient force is the conservative component of many types of forces exerted by light on particles. When it is derived from a potential, there is no heat transferred to the particle interacting with the light field. However, most theoretical descriptions of the gradient force use simplified configurations of the light field and particle interactions which overlook small amounts of heating. It is known that quantum fluctuations contribute to a very small but observable momentum diffusion of atoms and a corresponding increase in their temperature. This paper examines the contribution to momentum diffusion from a gradient force described as a quantum interaction between electron wave packets and a classical electromagnetic field. Stimulated transfers of photons between interfering light beams produce a small amount of heating that is difficult to detect in laboratory experiments. However the solar corona, with its thermal electrons irradiated by an intense electromagnetic field, provides ideal conditions for such a measurement. Heating from stimulated transfers contributes a large fraction of the observed coronal heating. Furthermore, the energy removed from the light field produces a wavelength shift of its spectrum as it travels through free electrons. Theory predicts a stimulated transfer redshift comparable to the redshift of distant objects observed in astronomy. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_02036 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Diffusive interactions between photons and electrons, an application to cosmology Marmet, L. Optics Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics The gradient force is the conservative component of many types of forces exerted by light on particles. When it is derived from a potential, there is no heat transferred to the particle interacting with the light field. However, most theoretical descriptions of the gradient force use simplified configurations of the light field and particle interactions which overlook small amounts of heating. It is known that quantum fluctuations contribute to a very small but observable momentum diffusion of atoms and a corresponding increase in their temperature. This paper examines the contribution to momentum diffusion from a gradient force described as a quantum interaction between electron wave packets and a classical electromagnetic field. Stimulated transfers of photons between interfering light beams produce a small amount of heating that is difficult to detect in laboratory experiments. However the solar corona, with its thermal electrons irradiated by an intense electromagnetic field, provides ideal conditions for such a measurement. Heating from stimulated transfers contributes a large fraction of the observed coronal heating. Furthermore, the energy removed from the light field produces a wavelength shift of its spectrum as it travels through free electrons. Theory predicts a stimulated transfer redshift comparable to the redshift of distant objects observed in astronomy. |
| title | Diffusive interactions between photons and electrons, an application to cosmology |
| topic | Optics Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2410.02036 |