Probability Current in the Relativistic Hamiltonian Quantum Mechanics

Probability Current in the Relativistic Hamiltonian Quantum Mechanics

Probability current in the relativistic Hamiltonian quantum mechanics Jakub Rembieli´nski University ofL´od´z Max Born Symposium, University of Wroc law, 28{30 June, 2011 Formulation of relativistic quantum mechanics: Salpeter equation K. Kowalski and J. Rembieli´nski,Salpeter equation and probability current in the relativistic Hamiltonian quantum mechanics (accepted for publication in Phys. Rev. A (2011)); continuation of: K. Kowalski and J. Rembieli´nski, The relativistic massless harmonic oscillator, Phys. Rev. A 81, 012118 (2010) p @ H = c2p2 + m2c4 + V (x); H ! i ; x ! x; p ! −i r ~@t ~ The spinless Salpeter equation: @ p i φ(x; t) = [ m2c4 − 2c2∆ + V (x)]φ(x; t) ~@t ~ L.L. Foldy, Synthesis of covariant particle equations, Phys. Rev. 102, 568 (1956) Probability current 2/27 Formulation of relativistic quantum mechanics: Salpeter equation K. Kowalski and J. Rembieli´nski,Salpeter equation and probability current in the relativistic Hamiltonian quantum mechanics (accepted for publication in Phys. Rev. A (2011)); continuation of: K. Kowalski and J. Rembieli´nski, The relativistic massless harmonic oscillator, Phys. Rev. A 81, 012118 (2010) p @ H = c2p2 + m2c4 + V (x); H ! i ; x ! x; p ! −i r ~@t ~ The spinless Salpeter equation: @ p i φ(x; t) = [ m2c4 − 2c2∆ + V (x)]φ(x; t) ~@t ~ L.L. Foldy, Synthesis of covariant particle equations, Phys. Rev. 102, 568 (1956) Probability current 2/27 Formulation of relativistic quantum mechanics: Salpeter equation K. Kowalski and J. Rembieli´nski,Salpeter equation and probability current in the relativistic Hamiltonian quantum mechanics (accepted for publication in Phys. Rev. A (2011)); continuation of: K. Kowalski and J. Rembieli´nski, The relativistic massless harmonic oscillator, Phys. Rev. A 81, 012118 (2010) p @ H = c2p2 + m2c4 + V (x); H ! i ; x ! x; p ! −i r ~@t ~ The spinless Salpeter equation: @ p i φ(x; t) = [ m2c4 − 2c2∆ + V (x)]φ(x; t) ~@t ~ L.L. Foldy, Synthesis of covariant particle equations, Phys. Rev. 102, 568 (1956) Probability current 2/27 Formulation of relativistic quantum mechanics: Salpeter equation K. Kowalski and J. Rembieli´nski,Salpeter equation and probability current in the relativistic Hamiltonian quantum mechanics (accepted for publication in Phys. Rev. A (2011)); continuation of: K. Kowalski and J. Rembieli´nski, The relativistic massless harmonic oscillator, Phys. Rev. A 81, 012118 (2010) p @ H = c2p2 + m2c4 + V (x); H ! i ; x ! x; p ! −i r ~@t ~ The spinless Salpeter equation: @ p i φ(x; t) = [ m2c4 − 2c2∆ + V (x)]φ(x; t) ~@t ~ L.L. Foldy, Synthesis of covariant particle equations, Phys. Rev. 102, 568 (1956) Probability current 2/27 Leslie L. Foldy (1919{2001) Probability current 3/27 Edwin E. Salpeter (1924{2008) Probability current 4/27 The Salpeter equation can be written in the form of the integro-differential equation @φ(x; t) Z i = d 3y K(x − y)φ(y; t) + V (x)φ(x; t) ~ @t where the kernel is given by 2 3 mc 2m c K2( jx − yj) K(x − y) = − ~ (2π)2~ jx − yj2 The Salpeter equation presumes the Newton-Wigner localization scheme implying the standard quantization rule x^ ! x, p^ ! −i~r. Consequently, the Hilbert space of solutions to the Salpeter is L2(R3; d 3x): Z hφj i = d 3x φ∗(x) (x) Therefore, we should identify jφ(x; t)j2 with the probability density ρ(x; t) satisfying the normalization condition: Z d 3x ρ(x; t) = 1 Probability current 5/27 The Salpeter equation can be written in the form of the integro-differential equation @φ(x; t) Z i = d 3y K(x − y)φ(y; t) + V (x)φ(x; t) ~ @t where the kernel is given by 2 3 mc 2m c K2( jx − yj) K(x − y) = − ~ (2π)2~ jx − yj2 The Salpeter equation presumes the Newton-Wigner localization scheme implying the standard quantization rule x^ ! x, p^ ! −i~r. Consequently, the Hilbert space of solutions to the Salpeter is L2(R3; d 3x): Z hφj i = d 3x φ∗(x) (x) Therefore, we should identify jφ(x; t)j2 with the probability density ρ(x; t) satisfying the normalization condition: Z d 3x ρ(x; t) = 1 Probability current 5/27 The Salpeter equation can be written in the form of the integro-differential equation @φ(x; t) Z i = d 3y K(x − y)φ(y; t) + V (x)φ(x; t) ~ @t where the kernel is given by 2 3 mc 2m c K2( jx − yj) K(x − y) = − ~ (2π)2~ jx − yj2 The Salpeter equation presumes the Newton-Wigner localization scheme implying the standard quantization rule x^ ! x, p^ ! −i~r. Consequently, the Hilbert space of solutions to the Salpeter is L2(R3; d 3x): Z hφj i = d 3x φ∗(x) (x) Therefore, we should identify jφ(x; t)j2 with the probability density ρ(x; t) satisfying the normalization condition: Z d 3x ρ(x; t) = 1 Probability current 5/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation possesses solutions of positive energies only and we have no problems with paradoxes occuring in the case of the Klein-Gordon equation I the agreement of predictions of the spinless Salpeter equation with the experimental spectrum of mesonic atoms is as good as for the Klein-Gordon equation I the Salpeter equation is widely used in the phenomenological description of the quark-antiquark-gluon system as a hadron model Probability current 6/27 The Salpeter equation was discarded because of: I its nonlocality I the lack of manifest Lorentz covariance However I the nonlocality of the Salpeter equation does not disturb the light cone structure 2 3 3 I the space L (R ; d x) of solutions to the Salpeter equation is invariant under the Lorentz group I the Salpeter equation

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    67 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us