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Abstract
We use the first-order approximate solutions to the nonlinear system of Klein-Gordon-Maxwell-Einstein equations describing the minimally coupled charged spin-less field to a spherically symmetric spacetime to analyze a becoming boson star. In the far future and long-range approximation, we derive an analytical time-dependent charge which allows us to point out several significant moments in the evolution of the boson nebula.
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Cite this article:
Ciprian Dariescu, Marina-Aura Dariescu. Boson Nebulae Charge[J]. Chin. Phys. Lett., 2010, 27(1): 011101. DOI: 10.1088/0256-307X/27/1/011101
Ciprian Dariescu, Marina-Aura Dariescu. Boson Nebulae Charge[J]. Chin. Phys. Lett., 2010, 27(1): 011101. DOI: 10.1088/0256-307X/27/1/011101
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Ciprian Dariescu, Marina-Aura Dariescu. Boson Nebulae Charge[J]. Chin. Phys. Lett., 2010, 27(1): 011101. DOI: 10.1088/0256-307X/27/1/011101
Ciprian Dariescu, Marina-Aura Dariescu. Boson Nebulae Charge[J]. Chin. Phys. Lett., 2010, 27(1): 011101. DOI: 10.1088/0256-307X/27/1/011101
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