Image of a regular phantom compact object and its luminosity under spherical accretions

Image of a regular phantom compact object and its luminosity under spherical accretions
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规则幻影致密天体的图像及其在球形吸积下的光度

DOI:
10.1088/1361-6382/abf712
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发表时间:
2020-11
期刊:
Class. Quantum Grav.
影响因子:
--
通讯作者:
荆继良
荆继良
中科院分区:
其他
文献类型:
--
作者:
秦欣;陈松柏;荆继良

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We have studied the shadow and its luminosity for a static and regular phantom compact object under the static spherical accretion and the infalling spherical accretion, respectively. Comparing with the usual Schwarzschild black hole, the presence of phantom hair yields the larger black hole shadow and the darker image. In both spherical accretion models, with the increase of phantom parameter, the maximum luminosity occurred at photon ring and the brightness of the central region in the shadow decrease, but in the region far from the shadow, the luminosity of image slightly increases. The image of a phantom wormhole and its luminosity have similar behaviors. Moreover, as the phantom charge parameter α increases up to the critical value at where the compact object changes from black hole to wormhole, there exists a jump for the specific intensity, which also appears in the slowly rotating case. This implies that the phantom hair is imprinted on both the shadow radius and the intensity of the electromagnetic flux radiation around compacted object.
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