25–28 May 2026
Albano Building 3
Europe/Stockholm timezone

Superluminal tunneling times in relativistic QFT

25 May 2026, 11:40
20m
Albano 3: 4204 - SU Conference Room (56 seats) (Albano Building 3)

Albano 3: 4204 - SU Conference Room (56 seats)

Albano Building 3

Hannes Alfvéns väg 12, 114 19 Stockholm
56

Speaker

Prof. Alex Matzkin (LPTM (CNRS and CY Cergy Paris Univ.))

Description

Many recent experimental works involving quantum tunneling claim their observations are consistent with superluminal or instantaneous barrier traversal times. However, we have recently proved [1] that microcausality prevents superluminal dynamics in the presence of tunneling in a QFT framework in which a potential barrier is represented by a background field. In this talk I will discuss how one can nevertheless define tunneling times that can in certain situations can give rise to superluminal velocities. I will focus on two such situations. First I will look at group velocities defined by connecting the maxima of the density expectation value to the left and to the right of a potential barrier [2]. A second example will involve working with a position operator of the Newton-Wigner type. The density is then propagated by the sole positive energy sector – evading microcausality and leading to densities leaking from the light cone [3]. For each case I will discuss the underlying physics (which turns out to be very different) and draw some lessons. [1] M. Alkhateeb and A. Matzkin, Phys. Rev. D 112, 076005, 2025 [2] D. Sokolovski and A. Matzkin, in preparation (should be posted on arxiv by mid-April) [3] F. Daem and A. Matzkin, Phys. Rev. A 111, L060202, 2025

Author

Prof. Alex Matzkin (LPTM (CNRS and CY Cergy Paris Univ.))

Presentation materials

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