Reconnection With Synchrotron Cooling And Pair Production

(PDF) Synchrotron Pair Production Equilibrium In Relativistic Magnetic Reconnection

(PDF) Synchrotron Pair Production Equilibrium In Relativistic Magnetic Reconnection We first compare how synchrotron cooling and pair production individually affect the overall dynamics of reconnection and the formation and evolution of plasmoids. We present the results of novel particle in cell simulations that track both the radiated synchrotron photons and the created pairs, with which we study the evolution of a two dimensional reconnecting current sheet in pair plasma.

(PDF) Synchrotron Pair Production Equilibrium In Relativistic Magnetic Reconnection

(PDF) Synchrotron Pair Production Equilibrium In Relativistic Magnetic Reconnection The simulations in this 2d/3d comparison study are conducted with the radiative pic code osiris, which self consistently accounts for the synchrotron radiation reaction on the emitting particles, and enables us to explore the effects of synchrotron cooling. We present the results of novel particle in cell simulations that track both the radiated synchrotron photons and the created pairs, with which we study the evolution of a two dimensional. We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization, σ, is high and the magnetic compactness, lb, of the system is of order unity. Magnetic reconnection is ubiquitous in astrophysical systems, and in many such systems the plasma suffers from significant cooling due to synchrotron radiation.

Synchrotron Emission | COSMOS

Synchrotron Emission | COSMOS We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization, σ, is high and the magnetic compactness, lb, of the system is of order unity. Magnetic reconnection is ubiquitous in astrophysical systems, and in many such systems the plasma suffers from significant cooling due to synchrotron radiation. We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization σ is high and the magnetic compactness ℓb of the system is of order unity. We present the results of 3d particle in cell simulations that explore relativistic magnetic reconnection in pair plasma with strong synchrotron cooling and a small mass fraction of nonradiating ions. We first compare how synchrotron cooling and pair production individually affect the overall dynamics of reconnection and the formation and evolution of plasmoids. We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization, σ, is high and the magnetic compactness, ℓb, of the system is of order unity.

Synchrotron Radiation From Prediction To Production | Request PDF

Synchrotron Radiation From Prediction To Production | Request PDF We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization σ is high and the magnetic compactness ℓb of the system is of order unity. We present the results of 3d particle in cell simulations that explore relativistic magnetic reconnection in pair plasma with strong synchrotron cooling and a small mass fraction of nonradiating ions. We first compare how synchrotron cooling and pair production individually affect the overall dynamics of reconnection and the formation and evolution of plasmoids. We study relativistic magnetic reconnection in the presence of strong synchrotron cooling, where the ambient magnetization, σ, is high and the magnetic compactness, ℓb, of the system is of order unity.

Reconnection with synchrotron cooling and pair production