Spectra of magnetic fields from electroweak symmetry breaking
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arXiv
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866916626769641472 |
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| author | Vachaspati, Tanmay Brandenburg, Axel |
| author_facet | Vachaspati, Tanmay Brandenburg, Axel |
| contents | We characterize magnetic fields produced during electroweak symmetry breaking by non-dynamical numerical simulations based on the Kibble mechanism. The generated magnetic fields were thought to have an energy spectrum $\propto k^3$ for small wavenumbers $k$, but here we show that it is actually a spectrum $\propto k^4$ along with characteristic fluctuations in the magnetic helicity. Using scaling results from MHD simulations for the evolution and assuming that the initial magnetic field is coherent on the electroweak Hubble scale, we estimate the magnetic field strength to be $\sim 10^{-13}\, \rmG$ on kpc scales at the present epoch for non-helical fields. For maximally helical fields we obtain $\sim 10^{-10}\, \rmG$ on Mpc scales. We also give scalings of these estimates for partially helical fields. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_00641 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Spectra of magnetic fields from electroweak symmetry breaking Vachaspati, Tanmay Brandenburg, Axel Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology We characterize magnetic fields produced during electroweak symmetry breaking by non-dynamical numerical simulations based on the Kibble mechanism. The generated magnetic fields were thought to have an energy spectrum $\propto k^3$ for small wavenumbers $k$, but here we show that it is actually a spectrum $\propto k^4$ along with characteristic fluctuations in the magnetic helicity. Using scaling results from MHD simulations for the evolution and assuming that the initial magnetic field is coherent on the electroweak Hubble scale, we estimate the magnetic field strength to be $\sim 10^{-13}\, \rmG$ on kpc scales at the present epoch for non-helical fields. For maximally helical fields we obtain $\sim 10^{-10}\, \rmG$ on Mpc scales. We also give scalings of these estimates for partially helical fields. |
| title | Spectra of magnetic fields from electroweak symmetry breaking |
| topic | Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2412.00641 |