- #36
James Essig
- 68
- 2
Hi GammaScanner;
I was sort of thinking gamma rays produced with an energy of rough order of magnitude of the temperature of the plasma in the form of black body radiation. The temperature of the plasma with nucleon/proton/other charged particles of about 10 EXP 15 K might very briefly radiate gamma rays on the order of 10 EXP 12 to 10 EXP 13 eV extrapolated from 1million to 10 million eV gamma rays from the initial plasma produced in the nanoseconds after the fusion sequence of a thermonuclear device is complete. A more realistic model might be the gamma ray energies that exist within the fission component just after the chain reaction has effectively ended. The maximum temperature of the fission reaction is about 100 million K at fission completion. For the fusion sequence, the maximum temperature reaches about 300 million to 400 million K although these temperatures are probably at locations well within the fusion stage where pressures and temperatures can be compounded by the compressive effects of the overlayers of fusioning material. At gamma ray energies approaching 1 TeV, interaction with quarks composing the nucleons no doubt becomes important.
Collisions of gamma rays among nucleons might produce some of the desired gamma rays through compton scattering, charged particle collisions might produce additional gamma rays, and other exotic reactions that produce extremely hard gamma rays such as those that occur in 1 TeV accellerators and soon, the 14 TeV accellator at the upgraded CERN may be gamma ray components. Although I would say that some way of producing a high enough plasma density would be required to allow for gamma ray interactions before the gamma rays would escape for compton scattering to work at these extreme energies.
Thanks for the insights and questions!
Regards;
Jim
I was sort of thinking gamma rays produced with an energy of rough order of magnitude of the temperature of the plasma in the form of black body radiation. The temperature of the plasma with nucleon/proton/other charged particles of about 10 EXP 15 K might very briefly radiate gamma rays on the order of 10 EXP 12 to 10 EXP 13 eV extrapolated from 1million to 10 million eV gamma rays from the initial plasma produced in the nanoseconds after the fusion sequence of a thermonuclear device is complete. A more realistic model might be the gamma ray energies that exist within the fission component just after the chain reaction has effectively ended. The maximum temperature of the fission reaction is about 100 million K at fission completion. For the fusion sequence, the maximum temperature reaches about 300 million to 400 million K although these temperatures are probably at locations well within the fusion stage where pressures and temperatures can be compounded by the compressive effects of the overlayers of fusioning material. At gamma ray energies approaching 1 TeV, interaction with quarks composing the nucleons no doubt becomes important.
Collisions of gamma rays among nucleons might produce some of the desired gamma rays through compton scattering, charged particle collisions might produce additional gamma rays, and other exotic reactions that produce extremely hard gamma rays such as those that occur in 1 TeV accellerators and soon, the 14 TeV accellator at the upgraded CERN may be gamma ray components. Although I would say that some way of producing a high enough plasma density would be required to allow for gamma ray interactions before the gamma rays would escape for compton scattering to work at these extreme energies.
Thanks for the insights and questions!
Regards;
Jim