Thomas-Wigner rotation as a holonomy for spin- 1/2 particles

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Veiko Palge
  • Christian Pfeifer

External Research Organisations

  • University of Tartu
  • Center of Applied Space Technology and Microgravity (ZARM)
View graph of relations

Details

Original languageEnglish
Article number032206
JournalPhysical Review A
Volume109
Issue number3
Publication statusPublished - 11 Mar 2024

Abstract

The Thomas-Wigner rotation (TWR) results from the fact that a combination of boosts leads to a nontrivial rotation of a physical system. Its origin lies in the structure of the Lorentz group. In this article we discuss the idea that the TWR can be understood in the geometric manner, being caused by the nontrivially curved relativistic momentum space, i.e., the mass shell, seen as a Riemannian manifold. We show explicitly how the TWR for a massive spin-1/2 particle can be calculated as a holonomy of the mass shell. To reach this conclusion we recall how to construct the spin bundle over the mass shell manifold. Interpreting TWR as a holonomy means it belongs to the same family of phenomena as Berry's phase.

ASJC Scopus subject areas

Cite this

Thomas-Wigner rotation as a holonomy for spin- 1/2 particles. / Palge, Veiko; Pfeifer, Christian.
In: Physical Review A, Vol. 109, No. 3, 032206, 11.03.2024.

Research output: Contribution to journalArticleResearchpeer review

Palge V, Pfeifer C. Thomas-Wigner rotation as a holonomy for spin- 1/2 particles. Physical Review A. 2024 Mar 11;109(3):032206. doi: 10.1103/PhysRevA.109.032206
Palge, Veiko ; Pfeifer, Christian. / Thomas-Wigner rotation as a holonomy for spin- 1/2 particles. In: Physical Review A. 2024 ; Vol. 109, No. 3.
Download
@article{4d6bf2a114b540159cdd30fdc81beaa2,
title = "Thomas-Wigner rotation as a holonomy for spin- 1/2 particles",
abstract = "The Thomas-Wigner rotation (TWR) results from the fact that a combination of boosts leads to a nontrivial rotation of a physical system. Its origin lies in the structure of the Lorentz group. In this article we discuss the idea that the TWR can be understood in the geometric manner, being caused by the nontrivially curved relativistic momentum space, i.e., the mass shell, seen as a Riemannian manifold. We show explicitly how the TWR for a massive spin-1/2 particle can be calculated as a holonomy of the mass shell. To reach this conclusion we recall how to construct the spin bundle over the mass shell manifold. Interpreting TWR as a holonomy means it belongs to the same family of phenomena as Berry's phase.",
author = "Veiko Palge and Christian Pfeifer",
note = "Publisher Copyright: {\textcopyright} 2024 American Physical Society.",
year = "2024",
month = mar,
day = "11",
doi = "10.1103/PhysRevA.109.032206",
language = "English",
volume = "109",
journal = "Physical Review A",
issn = "2469-9926",
publisher = "American Physical Society",
number = "3",

}

Download

TY - JOUR

T1 - Thomas-Wigner rotation as a holonomy for spin- 1/2 particles

AU - Palge, Veiko

AU - Pfeifer, Christian

N1 - Publisher Copyright: © 2024 American Physical Society.

PY - 2024/3/11

Y1 - 2024/3/11

N2 - The Thomas-Wigner rotation (TWR) results from the fact that a combination of boosts leads to a nontrivial rotation of a physical system. Its origin lies in the structure of the Lorentz group. In this article we discuss the idea that the TWR can be understood in the geometric manner, being caused by the nontrivially curved relativistic momentum space, i.e., the mass shell, seen as a Riemannian manifold. We show explicitly how the TWR for a massive spin-1/2 particle can be calculated as a holonomy of the mass shell. To reach this conclusion we recall how to construct the spin bundle over the mass shell manifold. Interpreting TWR as a holonomy means it belongs to the same family of phenomena as Berry's phase.

AB - The Thomas-Wigner rotation (TWR) results from the fact that a combination of boosts leads to a nontrivial rotation of a physical system. Its origin lies in the structure of the Lorentz group. In this article we discuss the idea that the TWR can be understood in the geometric manner, being caused by the nontrivially curved relativistic momentum space, i.e., the mass shell, seen as a Riemannian manifold. We show explicitly how the TWR for a massive spin-1/2 particle can be calculated as a holonomy of the mass shell. To reach this conclusion we recall how to construct the spin bundle over the mass shell manifold. Interpreting TWR as a holonomy means it belongs to the same family of phenomena as Berry's phase.

UR - http://www.scopus.com/inward/record.url?scp=85187540446&partnerID=8YFLogxK

U2 - 10.1103/PhysRevA.109.032206

DO - 10.1103/PhysRevA.109.032206

M3 - Article

AN - SCOPUS:85187540446

VL - 109

JO - Physical Review A

JF - Physical Review A

SN - 2469-9926

IS - 3

M1 - 032206

ER -