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Awaking the Vacuum in Relativistic Stars
(Amer Physical Soc, 2010-10-07)
Void of any inherent structure in classical physics, the vacuum has revealed to be incredibly crowded with all sorts of processes in relativistic quantum physics. Yet, its direct effects are usually so subtle that its ...
Awaking the Vacuum in Relativistic Stars
(Amer Physical Soc, 2010-10-07)
Void of any inherent structure in classical physics, the vacuum has revealed to be incredibly crowded with all sorts of processes in relativistic quantum physics. Yet, its direct effects are usually so subtle that its ...
Awaking the vacuum in relativistic stars
(2010-10-07)
Void of any inherent structure in classical physics, the vacuum has revealed to be incredibly crowded with all sorts of processes in relativistic quantum physics. Yet, its direct effects are usually so subtle that its ...
Gamma-ray emission from massive stars interacting with active galactic nuclei jets
(Oxford University Press, 2013-10)
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermassive black hole. In this work, we study the ...
Non-thermal emission from the interaction of extragalactic jets with stars
(AIP Publishing, 2017)
The central regions of galaxies are rich environments, with abundant stars and medium inhomogeneities. For galaxies hostingactive galactic nuclei, the interaction of a relativistic jet with obstacles can lead to the formation ...
From quantum to classical instability in relativistic stars
(Amer Physical Soc, 2015-01-07)
It has been shown that gravitational fields produced by realistic classical-matter distributions can force quantum vacuum fluctuations of some nonminimally coupled free scalar fields to undergo a phase of exponential growth. ...
From quantum to classical instability in relativistic stars
(2015-01-07)
It has been shown that gravitational fields produced by realistic classical-matter distributions can force quantum vacuum fluctuations of some nonminimally coupled free scalar fields to undergo a phase of exponential growth. ...