Are Black Holes sufficiently characterized?

In summary, the conversation discusses the necessary parameters for characterizing a black hole. The three main properties that are considered important are mass, angular momentum, and charge. However, there is also mention of entropy and surface area, which are derived from the three main properties. It is stated that for real black holes, the charge can be assumed to be zero, but all three parameters are needed for a complete description according to the no-hair theorem.
  • #1
cph
43
0
Is mass, angular momentum, and charge sufficient for black hole characterization? Or is also entropy, and hence surface area, also required? Thus is the shape for a given mass black hole also a required consideration?
 
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  • #2
From all the reading I've done, I gather that the mass and spin are the properties that matter. I haven't read of charge being much of an issue in real BHs and size seems to be mentioned only as the diameter of the event horizon.
 
  • #3
This is precisely the statement of the no-hair theorem, that mass, angular momentum, and charge are the only three numbers necessary to describe a BH. The quantities you mention, entropy and surface area, are derived from the above three.
 
  • #4
phinds said:
From all the reading I've done, I gather that the mass and spin are the properties that matter.
For real, astrophysical black-holes -- the charge can be assumed to be zero, as a black-hole will be formed from (ridiculously close to) equal numbers of protons and electrons. But all three parameters are actually needed for a complete description, as Nabeshin said---according to the http://en.wikipedia.org/wiki/No_hair_theorem"
 
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  • #5


I can say that the characterization of black holes is an ongoing and complex process. While the parameters of mass, angular momentum, and charge are certainly important in understanding black holes, they alone are not sufficient for complete characterization.

Entropy and surface area are also crucial factors in understanding black holes. The concept of entropy in black holes is closely tied to the second law of thermodynamics and plays a significant role in the study of black hole thermodynamics. The surface area of a black hole, also known as the event horizon, is directly related to its entropy, and thus, it is an essential consideration in characterizing these objects.

Moreover, the shape of a black hole is also an important factor to consider. While it is commonly believed that black holes are perfectly spherical, recent research suggests that they may have more complex shapes, such as oblate or prolate spheroids. The shape of a black hole can affect its gravitational pull and the dynamics of matter falling into it, making it a crucial consideration in characterization.

In conclusion, while mass, angular momentum, and charge are important parameters in characterizing black holes, entropy, surface area, and shape are also essential factors to consider. As scientists continue to study and understand these enigmatic objects, our understanding of their characterization will continue to evolve.
 

FAQ: Are Black Holes sufficiently characterized?

What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, including light, can escape from it. It is formed when a massive star dies and collapses in on itself, creating a singularity.

How do we detect black holes?

Black holes cannot be observed directly, but their presence can be inferred through their effects on surrounding matter and light. Scientists use various methods such as studying the behavior of stars and gas around the suspected black hole, observing gravitational lensing, and detecting X-rays emitted from the accretion disk around the black hole.

How do we characterize black holes?

Black holes are characterized by their mass, spin, and charge. The mass of a black hole can be estimated by observing its effect on surrounding objects. The spin and charge of a black hole can be inferred through mathematical models and observations of the surrounding matter and light.

Are all black holes the same?

No, black holes can vary in size, mass, and properties. There are primarily two types of black holes - stellar black holes, which are formed from the collapse of a massive star, and supermassive black holes, which are found at the center of most galaxies and are millions to billions of times more massive than the Sun.

Can black holes be dangerous to Earth?

No, black holes are typically very far away from Earth and do not pose any danger. However, if a black hole were to pass close enough to Earth, its strong gravitational pull could potentially disrupt the orbits of planets and other celestial bodies. But this scenario is highly unlikely to occur.

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