TY - JOUR

T1 - Spin and localization of relativistic fermions and uncertainty relations

AU - Céleri, Lucas C.

AU - Kiosses, Vasilis

AU - Terno, Daniel R.

N1 - CÃ©leri, Lucas C.; Kiosses, Vasilis and Terno, Daniel R. (2016). Spin and localization of relativistic fermions and uncertainty relations. Physical review A, 94(6), 062115. Copyright (2016) by the American Physical Society. The original article can be found at http://dx.doi.org/10.1103/PhysRevA.94.062115.

PY - 2016/12/19

Y1 - 2016/12/19

N2 - We discuss relations between several relativistic spin observables and derive a Lorentz-invariant characteristic of a reduced spin density matrix. A relativistic position operator that satisfies all the properties of its nonrelativistic analog does not exist. Instead we propose two causality-preserving positive operator-valued measures (POVMs) that are based on projections onto one-particle and antiparticle spaces, and on the normalized energy density. They predict identical expectation values for position. The variances differ by less than a quarter of the squared de Broglie wavelength and coincide in the nonrelativistic limit. Since the resulting statistical moment operators are not canonical conjugates of momentum, the Heisenberg uncertainty relations need not hold. Indeed, the energy density POVM leads to a lower uncertainty. We reformulate the standard equations of the spin dynamics by explicitly considering the charge-independent acceleration, allowing a consistent treatment of backreaction and inclusion of a weak gravitational field.

AB - We discuss relations between several relativistic spin observables and derive a Lorentz-invariant characteristic of a reduced spin density matrix. A relativistic position operator that satisfies all the properties of its nonrelativistic analog does not exist. Instead we propose two causality-preserving positive operator-valued measures (POVMs) that are based on projections onto one-particle and antiparticle spaces, and on the normalized energy density. They predict identical expectation values for position. The variances differ by less than a quarter of the squared de Broglie wavelength and coincide in the nonrelativistic limit. Since the resulting statistical moment operators are not canonical conjugates of momentum, the Heisenberg uncertainty relations need not hold. Indeed, the energy density POVM leads to a lower uncertainty. We reformulate the standard equations of the spin dynamics by explicitly considering the charge-independent acceleration, allowing a consistent treatment of backreaction and inclusion of a weak gravitational field.

UR - http://www.scopus.com/inward/record.url?scp=85006489311&partnerID=8YFLogxK

U2 - 10.1103/PhysRevA.94.062115

DO - 10.1103/PhysRevA.94.062115

M3 - Article

AN - SCOPUS:85006489311

SN - 2469-9926

VL - 94

SP - 1

EP - 11

JO - Physical Review A - Atomic, Molecular, and Optical Physics

JF - Physical Review A - Atomic, Molecular, and Optical Physics

IS - 6

M1 - 062115

ER -