Abstract:In the present work one-and two-photon pair production in a subcritical magnetic field have been considered. Two-photon production has been studied in the resonant case, when the cross section considerably increases compared to the nonresonant case. While one-photon pair production is considered to be the main mechanism of plasma generation in a pulsar magnetosphere, we suggest the existence of another one, which is resonant two-photon production process.Mod. Phys. Lett. A 30, 1550111 (2015); doi: http://dx
“…To evaluate the proportionality factor in Eq. ( 44), let us put the magnetic field equal to ℎ = 10 (such fields are observed near magnetars), the detuning to = 0.1, and the intermediate state width toΓ ∼ ℎ 2 [40]. Then the sought coefficient equals 0.1.…”
Section: Discussionmentioning
confidence: 99%
“…( 13) depend on ′ . Note that this propagator is widely used, when calculating the amplitudes of the second-order processes in which the electron plays the role of an intermediate particle (see, e.g., works [38][39][40]49]).…”
Section: Total Amplitude Of the − + Pair Photoproduction Taking The Polarization Loop Into Accountmentioning
confidence: 99%
“…Note also that, in the works [38,39], the resonant case of the process of electron-positron pair generation in a magnetic field by two photons was considered. In work [40], the 1 and resonant 2 pair creation processes were compared at the parameter values that are typical of the neutron star magnetosphere, and the limiting concentration of cyclotron photons at which the second-order process dominates over the first-order one was determined.…”
The process of the e−e+ pair photoproduction in a strong magnetic field through the polarization cascade (the creation of an e−e+ pair from a single photon and its subsequent annihilation to a single photon) has been considered. The kinematics of the process is analyzed, and the expression for the general amplitude is obtained. A radiation correction to the process of pair creation at the lowest Landau levels by a single photon is found in the case where the energy of this photon is close to the threshold value. A comparison with the process of e−e+ pair production by one photon is made.
“…To evaluate the proportionality factor in Eq. ( 44), let us put the magnetic field equal to ℎ = 10 (such fields are observed near magnetars), the detuning to = 0.1, and the intermediate state width toΓ ∼ ℎ 2 [40]. Then the sought coefficient equals 0.1.…”
Section: Discussionmentioning
confidence: 99%
“…( 13) depend on ′ . Note that this propagator is widely used, when calculating the amplitudes of the second-order processes in which the electron plays the role of an intermediate particle (see, e.g., works [38][39][40]49]).…”
Section: Total Amplitude Of the − + Pair Photoproduction Taking The Polarization Loop Into Accountmentioning
confidence: 99%
“…Note also that, in the works [38,39], the resonant case of the process of electron-positron pair generation in a magnetic field by two photons was considered. In work [40], the 1 and resonant 2 pair creation processes were compared at the parameter values that are typical of the neutron star magnetosphere, and the limiting concentration of cyclotron photons at which the second-order process dominates over the first-order one was determined.…”
The process of the e−e+ pair photoproduction in a strong magnetic field through the polarization cascade (the creation of an e−e+ pair from a single photon and its subsequent annihilation to a single photon) has been considered. The kinematics of the process is analyzed, and the expression for the general amplitude is obtained. A radiation correction to the process of pair creation at the lowest Landau levels by a single photon is found in the case where the energy of this photon is close to the threshold value. A comparison with the process of e−e+ pair production by one photon is made.
“…Later, it was found in works [25,26] using a slightly different method and in work [27] using precise solutions of the Dirac equation. It should be noted that this propagator was used in works [28][29][30][31] to calculate the amplitudes of second-order processes with the electron as an intermediate particle. The propagator has the form…”
Section: Electron Green's Function Via the Sum Over The Landau Levelsmentioning
confidence: 99%
“…In other words, the resonance condition is obeyed. In this case, the process width, which is usually associated with the total probability of the intermediate state decay [29][30][31], has to be taken into account. From expression (22), it is evident that the parameter˜plays the role of the resonance process width.…”
Section: Soft Photons and A Strong Magnetic Fieldmentioning
The birefringence effect in vacuum in strong magnetic fields has been considered. The polarization tensor in a constant external magnetic field is analyzed in the framework of quantum field theory and on the basis of the electron Green’s function calculated as the sum over the Landau levels. The case of the lowest Landau levels for photons with the energies below the electron-positron pair creation threshold is considered, and the corresponding refractive indices of the physical vacuum for anomalous and normal waves are determined.
The process of electron-positron pair production by a photon with subsequent annihilation to a single photon in a strong magnetic field has been studied. The general amplitude has been calculated and the process rate have been found in the low Landau levels approximation (resonant and nonresonant cases). The comparison of resonant and nonresonant cases shows a significant excess of the resonant rate. The polarization of the final photon in a strong magnetic field has also been found. It has been shown that polarizations of the initial and the final photons are independent except for the case of normal linear polarization of the initial photon.
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