47 research outputs found

    Radiation reaction in strong field QED

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    We derive radiation reaction from QED in a strong background field. We identify, in general, the diagrams and processes contributing to recoil effects in the average momentum of a scattered electron, using perturbation theory in the Furry picture: we work to lowest nontrivial order in the electromagnetic coupling alpha. For the explicit example of scattering in a plane wave background, we compare QED with classical electrodynamics in the limit h-bar goes to zero, finding agreement with the Lorentz-Abraham-Dirac and Landau-Lifshitz equations, and with Larmor's formula. The first quantum corrections are also presented.Comment: Version2: 7 pages, 2 figures. Discussion of related results and applications extended, references added. Matches version to appear in Phys.Lett.

    Radiation reaction from QED: lightfront perturbation theory in a plane wave background

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    We derive dynamical, real time radiation reaction effects from lightfront QED. Combining the Hamiltonian formalism with a plane wave background field, the calculation is performed in the Furry picture for which the background is treated exactly while interactions between quantum fields are treated in perturbation theory as normal. We work to a fixed order in perturbation theory, but no other approximation is made. The literature contains many proposals for the correct classical equation describing a radiating particle; we take the classical limit of our results and identify which equations are consistent with QED.Comment: 33 pages, 5 pdf figures. Version 3: corrected typographical mistakes and presentation issues in equations 4.10--4.14 and accompanying discussion. Results and conclusions unaffected and unchange

    Critical Schwinger pair production

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    We investigate Schwinger pair production in spatially inhomogeneous electric backgrounds. A critical point for the onset of pair production can be approached by fields that marginally provide sufficient electrostatic energy for an off-shell long-range electron-positron fluctuation to become a real pair. Close to this critical point, we observe features of universality which are analogous to continuous phase transitions in critical phenomena with the pair-production rate serving as an order parameter: electric backgrounds can be subdivided into universality classes and the onset of pair production exhibits characteristic scaling laws. An appropriate design of the electric background field can interpolate between power-law scaling, essential BKT-type scaling and a power-law scaling with log corrections. The corresponding critical exponents only depend on the large-scale features of the electric background, whereas the microscopic details of the background play the role of irrelevant perturbations not affecting criticality.Comment: 6 pages, 1 figur

    Quantum radiation reaction: Analytical approximations and obtaining the spectrum from moments

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    We derive analytical χ1\chi\ll1 approximations for spin-dependent quantum radiation reaction for locally constant and locally monochromatic fields. We show how to factor out fast spin oscillations and obtain the degree of polarization in the plane orthogonal to the magnetic field from the Frobenius norm of the Mueller matrix. We show that spin effects lead to a transseries in χ\chi, with powers χk\chi^k, logarithms (lnχ)k(\ln\chi)^k and oscillating terms, cos(/χ)\cos(\dots/\chi) and sin(/χ)\sin(\dots/\chi). In our approach we can obtain each moment, (kP)m\langle(kP)^m\rangle, of the lightfront longitudinal momentum independently of the other moments and without considering the spectrum. We show how to obtain a low-energy expansion of the spectrum from the moments by treating mm as a continuous, complex parameter and performing an inverse Mellin transform. We also show how to obtain the spectrum, without making a low-energy approximation, from a handful of moments using the principle of maximum entropy.Comment: 23 pages, 9 figure

    Momentum spectrum of nonlinear Breit-Wheeler pair production in space-time fields

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    We show how to use a worldline-instanton formalism to calculate, to leading order in the weak-field expansion, the momentum spectrum of nonlinear Breit-Wheeler pair production in fields that depend on time and one spatial coordinate. We find a nontrivial dependence on the width, λ\lambda, of the photon wave packet, and the existence of a critical point λc\lambda_c. For λ<λc\lambda<\lambda_c and a field with one peak, the spectrum has one peak where the electron and positron have the same energy. For λ>λc\lambda>\lambda_c this splits into two peaks. We calculate a high-energy (Ω1\Omega\gg1) expansion, which to leading order agrees with the results obtained by replacing the space-time field with a plane wave and using the well-known Volkov solutions. We also calculate an expansion for Ωa01\Omega\sim a_0\gg1, where the field is strong enough to significantly bend the trajectories of the fermions despite Ω1\Omega\gg1.Comment: 36 pages, 13 figure

    Plasma dynamics at the Schwinger limit and beyond

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    Strong field physics close to or above the Schwinger limit are typically studied with vacuum as initial condition, or by considering test particle dynamics. However, with a plasma present initially, quantum relativistic mechanisms such as Schwinger pair-creation are complemented by classical plasma nonlinearities. In this work we use the Dirac-Heisenberg-Wigner formalism to study the interplay between classical and quantum mechanical mechanisms for ultra-strong electric fields. In particular, the effects of initial density and temperature on the plasma oscillation dynamics are determined

    Worldline approach to helicity flip in plane waves

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    We apply worldline methods to the study of vacuum polarisation effects in plane wave backgrounds, in both scalar and spinor QED. We calculate helicity-flip probabilities to one loop order and treated exactly in the background field, and provide a toolkit of methods for use in investigations of higher-order processes. We also discuss the connections between the worldline, S-matrix, and lightfront approaches to vacuum polarisation effects.Comment: 11 pages, 1 figur
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