Covariance and noncovariance of relativistic spin equations

3 Jul 2024, 12:55
15m
Conference Hall (BLTP)

Conference Hall

BLTP

second floor, Chairman: Parfenov P.

Speaker

Alexander Silenko (Joint Institute for Nuclear Research)

Description

To solve difficult problems of nuclear spin physics like the proton spin crisis physicists should perfectly understand what spin is. There are a few correct definitions of the relativistic spin operators [1]: Dirac spin definition and two Foldy-Wouthuysen spin definitions coupled with the center-of-charge and center-of-mass position operators. The conventional definition explicitly or implicitly uses the Foldy-Wouthuysen representation and presents the total angular momentum as a sum of the orbital angular momentum defined in the laboratory frame and the spin defined in the particle rest frame. It has been proven [2] that this definition leads to noncovariant spin equations. Two other definitions result in covariant spin equations but are not convenient.

[1] Liping Zou, Pengming Zhang, and A. J. Silenko, Position and spin in relativistic quantum mechanics, Phys. Rev. A 101, 032117 (2020).

[2] A. A. Pomeransky, R. A. Senkov, and I. B. Khriplovich, Spinning relativistic particles in external fields, Usp. Fiz. Nauk 43, 1129 (2000) [Phys. Usp. 43, 1055 (2000)].

Section Nuclear structure: theory and experiment

Primary author

Alexander Silenko (Joint Institute for Nuclear Research)

Presentation materials