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100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

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144 R. H. Priceviscous heating <strong>of</strong> the gas which requires radiation for cooling. The details<strong>of</strong> the disk’s structure, temperature pr<strong>of</strong>ile, luminous signature, <strong>and</strong>so forth, all depend on the microphysics <strong>of</strong> the viscosity, <strong>and</strong> there is nosecure model for this. The viscosity may be based on the highly conductingplasma being threaded by tangled magnetic fields. In any case, somefeatures <strong>of</strong> the models are relatively insensitive to the details; one <strong>of</strong> theseis the nature <strong>of</strong> the characteristic radiation. Again it follows from a simpleorder-<strong>of</strong>-magnitude calculation that the temperature must be on theorder <strong>of</strong> 10 9 K, <strong>and</strong> the radiation will be predominately in the form <strong>of</strong>X-rays.When we move from stellar mass holes to supermassive holes, we movefrom physical models that miss details, to physical models themselves thatare still uncertain. But we also move to astrophysical black holes whoseexistence is essentially certain (or at least establishment dogma). Somegalaxies have active galactic nuclei (AGNs), tiny central regions that emitluminosity comparable to galactic luminosity, but are incredibly small onan astrophysical scale 13 . From a number <strong>of</strong> arguments, it is known thatthe engine – the source <strong>of</strong> energy – in these AGNs consists <strong>of</strong> a mass socompact that it must involve a supermassive black hole. The mechanism forproducing the radiation must certainly be different from that <strong>of</strong> a black holeaccretion disk, since AGNs are characterized by radio jets, narrow regions<strong>of</strong> strong radio emission emerging from a central source. Theorists believethat the mechanism for these complicated sources probably involves a largescale magnetic field anchored in a rapidly rotating supermassive hole. It isbelieved that this large scale magnetic field is created by the accretion <strong>of</strong>plasma carrying magnetic flux. The magnetic field then links the horizonto distant regions <strong>of</strong> the surrounding plasma. With the horizon playing therole <strong>of</strong> a rapidly rotating conducting membrane, the hole <strong>and</strong> magneticfield act like a kind <strong>of</strong> dynamo. The EMFs on rotating field lines createstrong currents that flow to the distant plasma linked by the field lines.The production <strong>of</strong> these currents, in effect, converts the rotational energy<strong>of</strong> the black hole into radio <strong>and</strong> other forms <strong>of</strong> radiation.There had been a distinct difference between the charactersitics <strong>and</strong>models <strong>of</strong> stellar mass holes <strong>and</strong> <strong>of</strong> supermassive holes, but a few yearsago this difference faded. A class <strong>of</strong> objects called “microquasars” 14 wasdiscovered that seemed to be stellar mass X-ray black holes that also havethe radio jets <strong>of</strong> AGNs. The tentative underst<strong>and</strong>ing <strong>of</strong> these microquasarsis that they are accretion disk objects that can build up large scale magneticfields <strong>and</strong> behave like AGNs scaled down by a linear factor <strong>of</strong> 10 8 or so.

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