We propose a new method to compute amplitudes of electroweak processes in the strong background magnetic field, using 7-+ e+e~ " as an example. We show that the moments of 7 —> • e + e ~ width are proportional to the derivatives of photon polarization function at the zero energy. Hence, the pair-production width can be easily calculated from the latter by the inverse Mellin transform. The prospects of our approach are commented. The electroweak phenomena associated with an intensive background magnetic field are rather rich. Under a background magnetic field, a physical photon can decay into an e+e~ ~ pair or split into two photons. Such processes are relevant to the attenuation of gamma-rays from pulsars1'2. Similarly, with a ...
The process of pair creation by a photon in a strong magnetic field is investigated basing on the po...
In this contribution, we present our recent compact master formulas for the multiphoton amplitudes o...
We calculate the neutrino self-energy operator Sigma (p) in the presence of a magnetic field B. In p...
We study the generation of strong magnetic fields in magnetars and in the early universe. For this p...
The problem of backreaction of quantum processes on the properties of the background field still rem...
This thesis is a study of the electrodynamic phenomena which can occur in strong magnetic fields (on...
In a strong magnetic field, a high-energy photon can be absorbed and then produce an electron-positr...
We reexamine the process $\gamma\to e^++ e^-$ in a background magnetic field comparable to $B_c\equi...
We develop the technique of inverse Mellin transform for processes occurring in a background magneti...
AbstractWe study the generation of strong magnetic fields in magnetars and in the early universe. Fo...
A new explicit analytical form of the dispersion relation for photon propagation in the presence of...
We propose a class of once-subtracted dispersion relations for the vacuum-polarization functions of ...
The literature review indicated the lack of a general Compton cross section for magnetic fields. An ...
Using a covariant photon propagator (developed by W. B. Campbell) to represent a photon exchange bet...
Using the quadratic expansion in the photon fields of Euler–Heisenberg (EH) non-linear electrodynami...
The process of pair creation by a photon in a strong magnetic field is investigated basing on the po...
In this contribution, we present our recent compact master formulas for the multiphoton amplitudes o...
We calculate the neutrino self-energy operator Sigma (p) in the presence of a magnetic field B. In p...
We study the generation of strong magnetic fields in magnetars and in the early universe. For this p...
The problem of backreaction of quantum processes on the properties of the background field still rem...
This thesis is a study of the electrodynamic phenomena which can occur in strong magnetic fields (on...
In a strong magnetic field, a high-energy photon can be absorbed and then produce an electron-positr...
We reexamine the process $\gamma\to e^++ e^-$ in a background magnetic field comparable to $B_c\equi...
We develop the technique of inverse Mellin transform for processes occurring in a background magneti...
AbstractWe study the generation of strong magnetic fields in magnetars and in the early universe. Fo...
A new explicit analytical form of the dispersion relation for photon propagation in the presence of...
We propose a class of once-subtracted dispersion relations for the vacuum-polarization functions of ...
The literature review indicated the lack of a general Compton cross section for magnetic fields. An ...
Using a covariant photon propagator (developed by W. B. Campbell) to represent a photon exchange bet...
Using the quadratic expansion in the photon fields of Euler–Heisenberg (EH) non-linear electrodynami...
The process of pair creation by a photon in a strong magnetic field is investigated basing on the po...
In this contribution, we present our recent compact master formulas for the multiphoton amplitudes o...
We calculate the neutrino self-energy operator Sigma (p) in the presence of a magnetic field B. In p...