JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling
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| Format: | Preprint |
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2024
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| _version_ | 1866917837152452608 |
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| author | Wang, Ze-Fan Lei, Lei Feng, Lei Fan, Yi-Zhong |
| author_facet | Wang, Ze-Fan Lei, Lei Feng, Lei Fan, Yi-Zhong |
| contents | It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe. Recently, James Webb Space Telescope (JWST) have released its early observations. In this work, we select the JWST spectroscopic observations of the high redshift ($z>7.1$) galaxies with strong [OIII] ($λ=4959$ Å\,and $5007$ Å\,in the rest frame) emission lines to constraint the evolution of the fine structure constant ($α$). With the spectra from two galaxies at redshifts of $7.19$ and $8.47$, the deviation of $α$ to its fiducial value is found to be as small as $0.44^{+8.4+1.7}_{-8.3-1.7} \times 10^{-4}$ and $-10.0^{+18+1.5}_{-18-1.5} \times 10^{-4}$, respectively (the first error is statistical and the latter is systematic). The combination of our results with the previous data reveals that $\frac{1}α \frac{d α}{dt} = 0.30^{+4.5}_{-4.5} \times 10^{-17}~{\rm yr^{-1}}$. Clearly, there is no evidence for a cosmic evolution of $α$. The prospect of further constraining the time evolution of $α$ is also discussed. The scalar field of dark energy is hypothesized to drive the acceleration of the universe's expansion through an interaction with the electromagnetic field. By integrating the observational data of the fine-structure constant variation, $\frac{Δα}α(z)$, we have established a stringent upper limit on the coupling strength between dark energy and electromagnetism. Our analysis yields $ζ\leq 3.92 \times 10^{-7}$ at the 95\% confidence level, representing the most stringent bound to date. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2411_08774 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling Wang, Ze-Fan Lei, Lei Feng, Lei Fan, Yi-Zhong Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe. Recently, James Webb Space Telescope (JWST) have released its early observations. In this work, we select the JWST spectroscopic observations of the high redshift ($z>7.1$) galaxies with strong [OIII] ($λ=4959$ Å\,and $5007$ Å\,in the rest frame) emission lines to constraint the evolution of the fine structure constant ($α$). With the spectra from two galaxies at redshifts of $7.19$ and $8.47$, the deviation of $α$ to its fiducial value is found to be as small as $0.44^{+8.4+1.7}_{-8.3-1.7} \times 10^{-4}$ and $-10.0^{+18+1.5}_{-18-1.5} \times 10^{-4}$, respectively (the first error is statistical and the latter is systematic). The combination of our results with the previous data reveals that $\frac{1}α \frac{d α}{dt} = 0.30^{+4.5}_{-4.5} \times 10^{-17}~{\rm yr^{-1}}$. Clearly, there is no evidence for a cosmic evolution of $α$. The prospect of further constraining the time evolution of $α$ is also discussed. The scalar field of dark energy is hypothesized to drive the acceleration of the universe's expansion through an interaction with the electromagnetic field. By integrating the observational data of the fine-structure constant variation, $\frac{Δα}α(z)$, we have established a stringent upper limit on the coupling strength between dark energy and electromagnetism. Our analysis yields $ζ\leq 3.92 \times 10^{-7}$ at the 95\% confidence level, representing the most stringent bound to date. |
| title | JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling |
| topic | Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2411.08774 |