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Malte F. Linder

Publications and source records attributed to Malte F. Linder.

4 recordsLinked to original sources

Condensed-matter analogs of the Sauter--Schwinger effect

The Sauter--Schwinger effect predicts the creation of electron--positron pairs from the vacuum due to a quasiconstant electric field $E_{\mathrm{strong}}$. The pair-creation yield can be exponentially enhanced without destroying the tunneling-like nature of this mechanism by adding a weaker temporal Sauter pulse $E_{\mathrm{weak}}/\cosh^{2}(ωt)$ with $ω$ above a certain threshold $ω_{\mathrm{crit}}$. In this original form of the so-called dynamically assisted Sauter--Schwinger effect, $ω_{\mathrm{crit}}$ is independent of $E_{\mathrm{weak}}\ll E_{\mathrm{strong}}$. Via the semiclassical solution (contour integral) of the Riccati equation in 1+1 spacetime dimensions, we find that a Gaussian-shaped pulse $E_{\mathrm{weak}}\exp[-(ωt)^{2}]$ assists tunneling in a similar way but with $ω_{\mathrm{crit}}$ depending on $E_{\mathrm{weak}}$. This remarkable sensitivity to the pulse shape arises due to the different pole structures of the vector potentials for complex times. We also study dynamical assistance by an oscillation $E_{\mathrm{weak}}\cos(ωt)$ as a model for counterpropagating laser beams and find another dependence $ω_{\mathrm{crit}}(E_{\mathrm{weak}})$. The largeness of the Schwinger limit $E_{\mathrm{crit}}^{\mathrm{QED}}\approx 10^{18}\,\mathrm{V/m}$ has rendered the observation of this nonperturbative pair-creation mechanism impossible so far. In order to facilitate a better understanding of this effect and its dynamical assistance via experiments, we propose an analog of the many-body Dirac Hamiltonian in direct-bandgap semiconductors. The nonrelativistic Bloch-electron Hamiltonian is restricted to the valence and conduction bands in reciprocal space, which correspond to the two relativistic energy continua. Similar models have been considered before---but mainly for constant external fields. [...]

hep-th

Analog Sauter-Schwinger effect in semiconductors for spacetime-dependent fields

The Sauter-Schwinger effect predicts the creation of electron-positron pairs out of the quantum vacuum via tunneling induced by a strong electric field. Unfortunately, as the required field strength is extremely large, this fundamental prediction of quantum field theory has not been verified experimentally yet. Here, we study under which conditions and approximations the interband tunneling in suitable semiconductors could be effectively governed by the same (Dirac) Hamiltonian, especially for electric fields which depend on space and time. This quantitative analogy would allow us to test some of the predictions (such as the dynamically assisted Sauter-Schwinger effect) in this area by means of these laboratory analogs.

cond-mat.mes-hall

Derivation of Hawking radiation in dispersive dielectric media

Motivated by recent experimental efforts, we study a black hole analog induced by the propagation of a strong laser pulse in a nonlinear dielectric medium. Based on the Hopfield model (one pair of Sellmeier coefficients), we perform an analytic and fully relativistic microscopic derivation of the analog of Hawking radiation in this setup. The Hawking temperature is determined by the analog of the surface gravity (as expected), but we also find a frequency-dependent gray-body factor (i.e., a nonthermal spectrum at infinity) due to the breaking of conformal invariance in this setup.

gr-qc

Pulse shape dependence in the dynamically assisted Sauter-Schwinger effect

While the Sauter-Schwinger effect describes nonperturbative electron-positron pair creation from vacuum by a strong and slowly varying electric field $E_{\mathrm{strong}}$ via tunneling, the dynamically assisted Sauter-Schwinger effect corresponds to a strong (exponential) enhancement of the pair-creation probability by an additional weak and fast electric or electromagnetic pulse $E_{\mathrm{weak}}$. Using the WKB and worldline instanton method, we find that this enhancement mechanism strongly depends on the shape of the fast pulse. For the Sauter profile $1/\cosh^2(ωt)$ considered previously, the threshold frequency $ω_{\mathrm{crit}}$ (where the enhancement mechanism sets in) is basically independent of the magnitude $E_{\mathrm{weak}}$ of the weak pulse---whereas for a Gaussian pulse $\exp(-ω^2t^2)$, an oscillating profile $\cos(ωt)$ or a standing wave $\cos(ωt)\cos(kx)$, the value of $ω_{\mathrm{crit}}$ does depend (logarithmically) on $E_{\mathrm{weak}}/E_{\mathrm{strong}}$.

hep-th