Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T22:37:57.693Z Has data issue: false hasContentIssue false
  • English
  • Français

Neutrino and γ-ray Emission from the Core of NGC1275 by Magnetic Reconnection: GRMHD Simulations and Radiative Transfer/Particle Calculations

Published online by Cambridge University Press:  07 April 2020

J. C. Rodríguez-Ramírez ,
Elisabete M. de Gouveia Dal Pino  and
R. Alves Batista
J. C. Rodríguez-Ramírez
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG-USP), Universidade de São Paulo. Cidade Universitaria R. do Matão, 1226 05508-090 São Paulo, SPBrasil email: [email protected]
Elisabete M. de Gouveia Dal Pino
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG-USP), Universidade de São Paulo. Cidade Universitaria R. do Matão, 1226 05508-090 São Paulo, SPBrasil email: [email protected]
R. Alves Batista
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG-USP), Universidade de São Paulo. Cidade Universitaria R. do Matão, 1226 05508-090 São Paulo, SPBrasil email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Very high energy (VHE) emission has been detected from the radio galaxy NGC1275, establishing it as a potential cosmic-ray (CR) accelerator and a high energy neutrino source. We here study neutrino and γ-ray emission from the core of NGC1275 simulating the interactions of CRs assumed to be accelerated by magnetic reconnection, with the accreting plasma environment. To do this, we combine (i) numerical general relativistic (GR) magneto-hydrodynamics (MHD), (ii) Monte Carlo GR leptonic radiative transfer and, (iii) Monte Carlo interaction of CRs. A leptonic emission model that reproduces the SED in the [103-1010.5] eV energy range is used as the background target for photo-pion interactions+electromagnetic cascading. CRs injected with the power-law index κ=1.3 produce an emission profile that matches the VHE tail of NGC1275. The associated neutrino flux, below the IceCube limits, peaks at ∼PeV energies. However, coming from a single source, this neutrino flux may be an over-estimation.

Keywords

galaxies: nucleiradiation mechanisms: non-thermalaccretionradiative transfer
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 184 - 188
Copyright
© International Astronomical Union 2020

References

Aartsen, M., Ackermann, M., Adams, J.et al. 2016, PhRvL 113, 101101Google Scholar
Abdo, A.et al. 2009, ApJ 699, 31CrossRefGoogle Scholar
Ackermann, M.et al. 2012, ApJS 203, 4CrossRefGoogle Scholar
Ajello, M.et al. 2009, ApJ 690, 367CrossRefGoogle Scholar
Aleksic, J.et al. 2012, A&A, 539L, 4Google Scholar
Aleksic, J.et al. 2012, A&A, 541, 99Google Scholar
Alves Batista, R., Dundovic, A., Erdmann, M., Kampert, K., Kuempel, D., Mller, G., Sigl, G., van Vliet, A., Walz, D. & Winchen, T. 2016, JCAP 05, 38CrossRefGoogle Scholar
de Gouveia Dal Pino, E. M.et al.These ProceedingsGoogle Scholar
de Gouveia Dal Pino, E. M. & Lazarian, A. 2005, A&A, 441, 845Google Scholar
de Gouveia Dal Pino, E. M., Piovezan, P. P. & Kadowaki, L. H. S. 2010a A&A, 518, A5CrossRefGoogle Scholar
Dolence, J., Gammie, C., Mościbrodzka & M, Leung, P-K 2009 ApJS, 184, 387DCrossRefGoogle Scholar
Gammie, C., McKinney, J., Toth, G. 2003, ApJ, 598, 444CrossRefGoogle Scholar
Johnstone, R. M. & Fabian, A. C. 1995, MNRAS, 273, 625CrossRefGoogle Scholar
Kadowaki, L. H. S., de Gouveia Dal Pino, E. M. & Singh, C. B. 2015, ApJ, 802, 113CrossRefGoogle Scholar
Kadowaki, L. H. S., de Gouveia Dal Pino, E. M. & Stone, J. 2018a, arXiv:1803.08557Google Scholar
Kadowaki, L. H. S., de Gouveia Dal Pino, E. M. & Stone, J. 2018b, In prep.Google Scholar
Kowal, G., de Gouveia Dal Pino, E. M. & Lazarian, A. 2011, ApJ, 735, 102CrossRefGoogle Scholar
Kowal, G., Dal Pino, de Gouveia & E. M., Lazarian, A. 2012, PhRvL, 108, 24Google Scholar
Lister, M. L., Aller, H. D., Aller, M. F.et al. 2009, AJ, 137, 3718CrossRefGoogle Scholar
Wilman, R., Edge, A., & Johnstone, R. 2005, MNRAS, 359, 755CrossRefGoogle Scholar