Abstract
Data obtained in the framework of the INTERBALL–Tail Probe (1995–2000) and RHESSI (from 2002 to the present) projects have revealed variations in the X-ray intensity of the solar corona in the photon energy range of 2−15 keV during the period of the quiet Sun. Previously, a hypothesis was proposed that this phenomenon could be associated with the effect of coronal heating. In the present study, a new mechanism of coronal plasma heating is proposed on the basis of the experimental data and the quantum theory of photon pairs that are produced from vacuum in the course of the Universe’s expansion. A similar mechanism based on the splitting of photon pairs in the interplanetary and intergalactic space is also proposed to explain the observed microwave background radiation.
Similar content being viewed by others
References
I. K. Mirzoeva, Astron. Lett. 31, 57 (2005).
I. K. Mirzoeva, Plasma Phys. Rep. 39, 316 (2013).
I. K. Mirzoeva, Plasma Phys. Rep. 44, 92 (2018).
A. Ringwald, Phys. Dark Univ 1, 116 (2012).
A. Ringwald, 25th Rencontres de Blois on Particle Physics and Cosmology, Blois, 2013. https://arxiv.org/pdf/1310.1256.pdf.
http://cast.web.cern.ch/CAST/.
K. Barth, A. Belov, B. Beltran, H. Bräuninger, J.M. Carmona, J. I. Collar, T. Dafni, M. Davenport, L. Di Lella, C. Eleftheriadis, J. Englhauser, G. Fanourakis, E. Ferrer-Ribas, H. Fischer, J. Franz, et al., J. Cosmol. Astropart. Phys., No. 5, 10 (2013).
F. J. Iguaz on behalf of the CAST Collaboration, 8th Symposium on Identification of Dark Matter, Montpellier, 2010. https://arxiv.org/pdf/1110.2116.pdf.
I. G. Irastorza, in Proceedings of Symposium on Detector Developments for Particle, Astroparticle, and Synchrotron Radiation Experiments, Stanford, CA, 2006.
G. W. Fraser, A. M. Read, S. Sembay, J. A. Carter, and E. Schyns, Potential solar axion signatures in X-ray observations with the XMM-Newton observatory, 2014. https://arxiv.org/ftp/arxiv/papers/1403/1403.2436.pdf.
S. G. Chefranov and E. A. Novikov, JETP 111, 731 (2010).
E. A. Novikov, Vacuum response to cosmic stretching: accelerated Universe and prevention of singularity, 2006. https://arxiv.org/pdf/nlin/0608050.pdf.
E. B. Gliner, Sov. Phys. JETP 22, 378 (1966).
E. B. Gliner, Sov. Phys. Doklady 15, 559 (1970).
A. D. Sakharov, Sov. Phys. Doklady 12, 1040 (1967).
A. A. Starobinskii, Sov. Astron. Lett. 4, 82 (1978).
E. A. Novikov, Mod. Phys. Lett. A 31, 1650092 (2016).
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © I.K. Mirzoeva, S.G. Chefranov, 2018, published in Fizika Plazmy, 2018, Vol. 44, No. 10, pp. 791–797.
Rights and permissions
About this article
Cite this article
Mirzoeva, I.K., Chefranov, S.G. Variations in the X-ray Intensity of the Solar Corona and Heating of the Coronal Plasma in the Context of the Quantum Theory of Photon Pairs. Plasma Phys. Rep. 44, 920–925 (2018). https://doi.org/10.1134/S1063780X18100094
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063780X18100094