尘埃崩在非对称安全:通往常规黑洞的道路
Alfio Bonanno1, Daniele Malafarina2, Antonio Panassiti3
1INAF, Osservatorio Astrofisico di Catania, via S.Sofia 78, I-95123 Catania, Italy and INFN, Sezione di Catania, via S.Sofia 64, I-95123 Catania, Italy.
Physical review letters
|February 2, 2024
概括
这项研究提出了正规黑洞的新模型,表明它们可以通过引力崩而没有奇点形成. 不对称的安全引力确保了黑洞的存在.
科学领域:
- 理论物理学的理论物理.
- 量子引力是一种量子引力.
- 黑洞物理学 黑洞物理学
背景情况:
- 黑洞通常是由包含奇点的时空描述的.
- 了解黑洞的形成和内部需要量子引力方法.
研究的目的:
- 用量子爱因斯坦引力构建正规的黑洞时空.
- 调查物质-几何相互作用在避免奇点中的作用.
主要方法:
- 从量子爱因斯坦引力的有效拉格朗推导出正规黑洞时空.
- 将内部物质建模为具有乘法合功能的尘液 (χ).
- 从异常安全的重力推导出 χ,假设物质对罗伊特固定点的影响最小.
主要成果:
- 在高能量的情况下,引力合会消失.
- 静态外形几何是由交叉条件决定的.
- 由此产生的时空几何在任何时候都是无奇点的.
结论:
- 这个模型提供了通过引力崩形成正规黑洞的机制.
- 无奇点的性质来自于在非对称的安全引力中的特定物质-几何相互作用.
相关概念视频
Schwarzschild Radius and Event Horizon
2.0K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.0K
Detection of Black Holes
2.2K
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
2.2K
Space-Time Curvature and the General Theory of Relativity
2.7K
In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of...
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of...
2.7K
Conservation of Mass in Finite Cotrol Volume
1.3K
The principle of conservation of mass is a fundamental law in fluid mechanics and is applied using the continuity equation. We apply the concept to a finite control volume to derive the continuity equation.
A system is defined as a collection of unchanging contents, and the conservation of mass states that a system's mass is constant.
A system is defined as a collection of unchanging contents, and the conservation of mass states that a system's mass is constant.
1.3K
Conservation of Angular Momentum: Application
10.9K
A system's total angular momentum remains constant if the net external torque acting on the system is zero. Examples of such systems include a freely spinning bicycle tire that slows over time due to torque arising from friction, or the slowing of Earth's rotation over millions of years due to frictional forces exerted on tidal deformations. However in the absence of a net external torque, the angular momentum remains conserved. The conservation of angular momentum principle requires a...
10.9K
First Law: Particles in One-dimensional Equilibrium
6.9K
Newton's first law of motion states that a body at rest remains at rest, or if in motion, remains in motion at constant velocity, unless acted on by a net external force. It also states that there must be a cause for any change in velocity (a change in either magnitude or direction) to occur. This cause is a net external force. For example, consider what happens to an object sliding along a rough horizontal surface. The object quickly grinds to a halt, due to the net force of friction. If...
6.9K


