Black Holes: X-rays, Gamma Rays & Light Emission

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Discussion Overview

The discussion revolves around the mechanisms by which black holes are associated with emissions of X-rays, gamma rays, and light, particularly focusing on the nature of these emissions in relation to the event horizon and gravitational effects. The scope includes theoretical considerations, observational implications, and speculative radiation phenomena.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions how X-rays and gamma rays can escape a black hole's event horizon, referencing a claim from "Brief History of Time" about light emission at the boundary.
  • Another participant suggests that X-rays are generated by a superheated accretion disk around the black hole, where material falling in loses potential energy and heats up, emitting X-rays before crossing the event horizon.
  • A different viewpoint introduces the concept of Hawking radiation, stating that black holes can emit faint radiation detectable by observers, although this is described as speculative and dependent on theoretical frameworks not yet fully established.
  • One participant raises a question about how X-rays reach Earth, suggesting the role of space observatories and sensitive Earth-based observatories, indicating a potential misunderstanding of the original question regarding black holes.

Areas of Agreement / Disagreement

Participants express differing views on the mechanisms of emission related to black holes, with some focusing on accretion disks while others introduce Hawking radiation. The discussion remains unresolved regarding the specifics of how emissions escape gravitational influence.

Contextual Notes

The discussion includes speculative elements, particularly regarding Hawking radiation, which relies on theoretical constructs that are not universally accepted. There are also assumptions about the nature of emissions and their detection that are not fully explored.

Who May Find This Useful

Readers interested in astrophysics, black hole physics, and the observational aspects of high-energy emissions may find this discussion relevant.

Pakbabydoll
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IF nothing can escape from a black hole's event horizon,
then how do x-rays and Gamma rays escape? and how does it emits light?
it says in "Brief History of Time" that the light it emits is just at the boundary of the event horizon. So then how does it escape the gravity and reach earth? (x-rays) since Gamma rays can't get through the atmosphere. :rolleyes:
 
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In most cases it will be a superheated accretion disk that is generating the X-ray emmisions. As you can imagine when somehing falls toward a black hole it loses an enormous amount of potential energy and this will heat an accretion disk to the point where it emits x-rays. Black holes do not emit light, but stuff that has not crossed the event horizon can.

You may find the following link interesting as it has a lot of information about X-ray binaries.

http://imagine.gsfc.nasa.gov/docs/science/know_l2/binaries.html
 
Even a black hole without accretion disk will emmit extremely faint radiation - the so called Hawking radiation. It is a speculative quantum calculation first done by Hawking showing that the observer at infinity detects flux of particles coming from the black hole. The flux was formed during the formation of the black hole just outside its horizon.

An eternal black hole (not formed by collapse of matter) doesn't emmit Hawking radiation.

The calculation is speculative because it was done in a 'semiclassical approximation' to Quantum gravity, a theory yet to be created.
 
Pakbabydoll said:
So then how does it escape the gravity and reach earth? (x-rays) since Gamma rays can't get through the atmosphere. :rolleyes:
Space observatories? Sensitive, Earth-based observatories? This seems an unrelated question to your first one about BHs.
 

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