Relativistic Gamow Vectors
A. Bohm, H. Kaldass, S. Wickramasekara, P. Kielanowski
Abstract
Gamow vectors in non-relativistic quantum mechanics are generalized eigenvectors (kets) of self-adjoint Hamiltonians with complex eigenvalues. Like the Dirac kets, they are mathematically well defined in the Rigged Hilbert Space. Gamow kets are derived from the resonance poles of the S-matrix. They have a Breit-Wigner energy distribution, an exponential decay law, and are members of a basis vector expansion whose truncation gives the finite dimensional effective theories with a complex Hamiltonian matrix. They also have an asymmetric time evolution described by a semigroup generated by the Hamiltonian, which expresses a fundamental quantum mechanical arrow of time. These Gamow kets are generalized to relativistic Gamow vectors by extrapolating from the Galilei group to the Poincare group. This leads to semigroup representations of the Poincare group which are characterized by spin j and complex invariant mass square. In these non-unitary representations the Lorentz subgroup is unitarily represented and the four-momenta are "minimally complex" in the sense that the four-velocity is real. The relativistic Gamow vectors have all the properties listed above for the non-relativistic Gamow vectors and are therefore ideally suited to describe relativistic resonances and quasistable particles.
Create a lesson
Related papers
Horizon exchange and the universal all-spin response of Kerr
Pierre Vanhove
Hecke Relations from Self-Duality
Justin Kaidi
Weyl Rescalings: A First Order Approach
L. Andrianopoli, J. Zanelli
Interpolating between 4d N= 1 SCFT supercurrent multiplet anomalies
Pantelis Panopoulos, Ioannis Papadimitriou
Crossover from Schwarzian dynamics to rotational soft modes in near-extremal Lovelock black holes
Ankit Anand, Aditya Singh, Kimet Jusufi
Fortuitous BMN Operators from Multiple Cores
Robert de Mello Koch, Sarthak Duary, Minkyoo Kim et al.