论文标题
{\ bf k-} Essence Emperent vaidya spacetime中的霍金温度蒸发的动力视野蒸发
Evaporation of dynamical horizon with the Hawking temparature in the {\bf K-}essence emergent Vaidya spacetime
论文作者
论文摘要
在{\ bf k-} Essence vaidya schwarzschild时空中，我们应用动态范围方程来测量由于鹰辐射和隧道形式主义（Hamilton-Jacobi方法）引起的大规模损失，以计算鹰温度。假设在这里{\ bf k-}本质的狄拉克出生的智能动作是一种非标准动作，那么背景物理时空是一个静态的球形对称黑洞，我们仅限于{\ bf k-}本质标量场仅是向前或向后时间的函数。 {\ bf k-}本质紧急引力和Vaidya时空的概括已由Manna等人联系起来。在本文中，我们使用Sawayama对动态视野的修改描述，以表明所获得的发现偏离了标准的Vaidya时空几何形状。
In the {\bf K-}essence Vaidya Schwarzschild spacetime, we apply the dynamical horizon equation to measure the mass-loss due to Hawking radiation and the tunneling formalism (Hamilton-Jacobi method) to calculate the hawking temperature. Assuming the Dirac-Born-Infeld kind of non-standard action for the {\bf K-}essence here, the background physical spacetime is a static spherically symmetric black hole, and we constrain the {\bf K-}essence scalar field to be a function only of either forward or backward time. The {\bf K-}essence emergent gravity and the generalizations of Vaidya spacetime have been linked by Manna et al. In this paper, we use Sawayama's modified description of the dynamical horizon to show that the obtained findings deviate from the standard Vaidya spacetime geometry.
