scholarly journals Probing nonlinear electrodynamics in slowly rotating spacetimes through neutrino astrophysics

2017 ◽  
Vol 95 (2) ◽  
Author(s):  
Herman J. Mosquera Cuesta ◽  
Gaetano Lambiase ◽  
Jonas P. Pereira
2014 ◽  
Vol 29 (21) ◽  
pp. 1444010
Author(s):  
Bruce H. J. McKellar ◽  
T. J. Goldman ◽  
G. J. Stephenson

If fermions interact with a scalar field, and there are many fermions present the scalar field may develop an expectation value and generate an effective mass for the fermions. This can lead to the formation of fermion clusters, which could be relevant for neutrino astrophysics and for dark matter astrophysics. Because this system may exhibit negative pressure, it also leads to a model of dark energy.


2016 ◽  
Vol 94 (4) ◽  
Author(s):  
V. I. Denisov ◽  
B. N. Shvilkin ◽  
V. A. Sokolov ◽  
M. I. Vasili’ev

2013 ◽  
Vol 474 ◽  
pp. 012023 ◽  
Author(s):  
E Ivanov ◽  
O Lechtenfeld ◽  
B Zupnik

2005 ◽  
Vol 20 (11) ◽  
pp. 2421-2430 ◽  
Author(s):  
M. NOVELLO

We present some consequences induced by nonlinear electrodynamics on the global properties of the universe.


2021 ◽  
pp. 2150137
Author(s):  
Shahid Chaudhary ◽  
Abdul Jawad ◽  
Kimet Jusufi ◽  
Muhammad Yasir

This paper explores the influence of special type of higher order generalized uncertainty principle on the thermodynamics of five-dimensional black hole in Einstein–Gauss–Bonnet gravity coupled to nonlinear electrodynamics. We examine the corrected thermodynamical properties of the black hole with some interesting limiting cases [Formula: see text] and [Formula: see text] and compared our results with usual thermodynamical relations. We observe that the influence of GUP correction stabilizes the BH and BH solution remains physical throughout the region of horizon radius. In this framework, we also uncover the relationship of shadow radius and quasinormal modes of the mentioned black hole. We conclude that shadow radius of our considered black hole is a perfect circle and it decreases with increasing values of charge and Gauss–Bonnet parameter. We also verify the inverse relation between the quasinormal modes frequencies and shadow radius, i.e. quasinormal modes should increase with increasing values of Gauss–Bonnet parameter and electric charge.


2017 ◽  
Vol 529 (8) ◽  
pp. 1700073 ◽  
Author(s):  
S. I. Kruglov

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