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Relativistic Jets from Supermassive Black Holes? |
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| Jul2-12, 04:15 AM | #1 |
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Relativistic Jets from Supermassive Black Holes?
If nothing can escape black holes, how are relativistic jets of particles and radiation emitted from the supermassive variety of the same? Are they emitted from the BH proper or from something else?
IH |
| Jul2-12, 04:42 AM | #2 |
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See post number 13 in this thread: http://www.physicsforums.com/showthread.php?t=223661
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| Jul2-12, 04:52 AM | #3 |
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Thanx for the reference; so it remains something of a 'mystery'. Perhaps one thing that can be said is that if the jets are not emitted from the BH proper -and classic BH theory would preclude that- they must be emitted from the accretion disk. I fail to see by what possible mechanism though. It just seems impossible even to speculate as to how this may be achieved... Faro |
| Jul2-12, 04:59 AM | #4 |
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Relativistic Jets from Supermassive Black Holes?
Discussion as to the possible ways of emission shouldn't be a problem. Inventing your own theory based on little to no evidence or understanding of astrophysics and other related areas would be a very big problem and would be against PF rules. As I like to put it, asking questions is fine. Proposing solutions isn't. Those are for papers and peer review.
The particles must almost assuredly come from the accretion disk initially, as they wouldn't be able to escape from beyond the event horizon. I believe that a similar problem with the jets from neutron stars exists as well. Perhaps they occur for the same reasons. |
| Jul2-12, 05:17 AM | #5 |
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I wonder is there any evidence as to how the jet forms initially? Do we know for example whether the initial jet (presumably emitted from the accretion disk) is cylindrical or conic in shape? Do we have sufficient resolution in imaging to do this? IH |
| Jul2-12, 05:35 AM | #6 |
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| Jul2-12, 09:46 AM | #7 |
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Indeed, the emission is often seen to be conical. A helical structure is often seen on large scales, though, for example in 3C 273 and S5 0835+710:
Anatomy of Helical Extragalactic Jets: The Case of S5 0836+710 I haven't sifted through too much of the literature on the structure of jets proper, but the helical structure is often thought to be due to some periodic process like possible precession of the source of the jet, which is assumed to be the accretion disk. The disk amplifies any magnetic field and twists and collimates the field along the axis of rotation. The wiki article on relativistic jets, while short, mentions a couple of mechanisms, though is not an exhaustive review. |
| Jul2-12, 12:14 PM | #8 |
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Would it be easier to propose a mechanism if the jets were composed of radiation only without any massive particles? Can we today somehow simulate a 'mini-accretion disk' in the laboratory? IH |
| Jul2-12, 12:49 PM | #9 |
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| Jul2-12, 01:28 PM | #10 |
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But then one would expect to have two jets jutting out from opposite poles of a BH/accretion disk, one with positively charged particles and another with negatively charged particles. How then does one explain single-jet occurrences like in this pic: http://en.wikipedia.org/wiki/File:Onde-radioM87.jpg IH |
| Jul2-12, 03:34 PM | #11 |
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M87 has evidence of an antipodal jet, I believe. The one-sided jet is typically explained away as a relativistic effect, due to beaming:
http://en.wikipedia.org/wiki/Relativistic_beaming Basically, there just isn't enough light being emitted towards us to be seen with previous observations. Special relativity also explains the observed apparent superluminal motion seen in some of these jets, M87 included: http://en.wikipedia.org/wiki/Superluminal_motion |
| Jul2-12, 03:43 PM | #12 |
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| Jul2-12, 04:41 PM | #13 |
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Very interesting that the two proposed mechanisms in the wiki article both involve energy transfer from the BH to the jet. What about mass-energy equivalence? Energy may escape from a BH but not mass? But then photons are massless and they cannot escape either...very confusing... IH |
| Jul2-12, 05:14 PM | #14 |
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Nothing is escaping the event horizon, the particles and energy observed orginate outside the event horizon.
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