A phase-resolved Fermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere
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arXiv
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| Autori principali: | , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866910364519628800 |
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| author | Fiori, A. Razzano, M. Harding, A. K. Kerr, M. Mignani, R. P. Parkinson, P. M. Saz |
| author_facet | Fiori, A. Razzano, M. Harding, A. K. Kerr, M. Mignani, R. P. Parkinson, P. M. Saz |
| contents | The goal of our work is to study the mode changes of the radio-quiet gamma-ray pulsar PSR J2021+4026 with improved detail. By accurately characterizing variations in the gamma-ray spectrum and pulse profile, we aim to relate the Fermi-LAT observations to theoretical models and interpret the mode changes in terms of variations in the structure of a multipolar dissipative magnetosphere. We continually monitored the rotational evolution and the gamma-ray flux of PSR J2021+4026 using more than 13 years of Fermi-LAT data with a binned likelihood approach. We clearly detect the previous mode changes and confirm a more recent mode change that occurred around June 2020. We investigated the features of the phase-resolved spectrum and pulse profile, and we inferred the macroscopic conductivity, the electric field parallel to the magnetic field, and the curvature radiation cutoff energy. These physical quantities are related to the spin-down rate and the gamma-ray flux and therefore are relevant to the theoretical interpretation of the mode changes. We computed the relative variations in the best-fit parameters, finding typical flux changes between 13% and 20%. Correlations appear between the gamma-ray flux and the spectral parameters, as the peak of the spectrum shifts by about 10% toward lower energies when the flux decreases. The analysis of the pulse profile reveals that the pulsed fraction of the light curve is larger when the flux is low. We introduced a simple magnetosphere model that combines a dipole field with a strong quadrupole component. We simulated magnetic field configurations to determine the positions of the polar caps for different sets of parameters, and we conclude that some configurations could explain the observed multiwavelength variability. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_07649 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A phase-resolved Fermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere Fiori, A. Razzano, M. Harding, A. K. Kerr, M. Mignani, R. P. Parkinson, P. M. Saz High Energy Astrophysical Phenomena The goal of our work is to study the mode changes of the radio-quiet gamma-ray pulsar PSR J2021+4026 with improved detail. By accurately characterizing variations in the gamma-ray spectrum and pulse profile, we aim to relate the Fermi-LAT observations to theoretical models and interpret the mode changes in terms of variations in the structure of a multipolar dissipative magnetosphere. We continually monitored the rotational evolution and the gamma-ray flux of PSR J2021+4026 using more than 13 years of Fermi-LAT data with a binned likelihood approach. We clearly detect the previous mode changes and confirm a more recent mode change that occurred around June 2020. We investigated the features of the phase-resolved spectrum and pulse profile, and we inferred the macroscopic conductivity, the electric field parallel to the magnetic field, and the curvature radiation cutoff energy. These physical quantities are related to the spin-down rate and the gamma-ray flux and therefore are relevant to the theoretical interpretation of the mode changes. We computed the relative variations in the best-fit parameters, finding typical flux changes between 13% and 20%. Correlations appear between the gamma-ray flux and the spectral parameters, as the peak of the spectrum shifts by about 10% toward lower energies when the flux decreases. The analysis of the pulse profile reveals that the pulsed fraction of the light curve is larger when the flux is low. We introduced a simple magnetosphere model that combines a dipole field with a strong quadrupole component. We simulated magnetic field configurations to determine the positions of the polar caps for different sets of parameters, and we conclude that some configurations could explain the observed multiwavelength variability. |
| title | A phase-resolved Fermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2403.07649 |