Lorentz covariant physical Brownian motion: Classical and quantum
In this work, we re-examine the Goldstein-Kaç (also called Poisson-Kaç) velocity switching model from two points of view. On the one hand, we prove that the forward and backward Chapman–Kolmogorov equations of the stochastic process are Lorentz covariant when the trajectories are parameterized by th...
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Published in | Annals of physics Vol. 472; p. 169857 |
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Language | English |
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ISSN | 0003-4916 |
DOI | 10.1016/j.aop.2024.169857 |
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Abstract | In this work, we re-examine the Goldstein-Kaç (also called Poisson-Kaç) velocity switching model from two points of view. On the one hand, we prove that the forward and backward Chapman–Kolmogorov equations of the stochastic process are Lorentz covariant when the trajectories are parameterized by their proper time. On the other hand, to recast the model as a quantum random evolution, we restate the Goldstein-Kaç model as a Hamiltonian system, which can then be quantized using the standard correspondence rules. It turns out that the density matrix for the random quantum evolution satisfies a Chapman–Kolmogorov equation similar to that of the classical case, and therefore, it is also Lorentz covariant. To finish, we verify that the quantum model is also consistent with special relativity and that transitions outside the light cone, that is, transitions between states with disjoint supports in space–time, cannot occur. |
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AbstractList | In this work, we re-examine the Goldstein-Kaç (also called Poisson-Kaç) velocity switching model from two points of view. On the one hand, we prove that the forward and backward Chapman–Kolmogorov equations of the stochastic process are Lorentz covariant when the trajectories are parameterized by their proper time. On the other hand, to recast the model as a quantum random evolution, we restate the Goldstein-Kaç model as a Hamiltonian system, which can then be quantized using the standard correspondence rules. It turns out that the density matrix for the random quantum evolution satisfies a Chapman–Kolmogorov equation similar to that of the classical case, and therefore, it is also Lorentz covariant. To finish, we verify that the quantum model is also consistent with special relativity and that transitions outside the light cone, that is, transitions between states with disjoint supports in space–time, cannot occur. |
ArticleNumber | 169857 |
Author | Gzyl, Henryk |
Author_xml | – sequence: 1 givenname: Henryk orcidid: 0000-0002-3781-8848 surname: Gzyl fullname: Gzyl, Henryk email: henryk.gzyl@iesa.edu.ve organization: Centro de Finanzas IESA, Caracas, Venezuela |
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Cites_doi | 10.3934/mbe.2019171 10.1103/PhysRevE.71.016124 10.1073/pnas.1717292115 10.1016/S0378-4371(02)00805-1 10.1088/1751-8121/acf1e0 10.1007/s10955-024-03284-x 10.1007/BF02083813 10.1093/qjmam/4.2.129 10.1007/s11128-013-0603-z 10.3390/e24020201 10.1016/0003-4916(91)90045-A 10.1103/PhysRevE.96.042133 10.1216/RMJ-1974-4-3-497 10.1140/epjb/e2017-80123-7 10.1209/0295-5075/126/50001 10.1007/BF02190048 10.1017/S0021900200047707 10.1016/0378-4371(89)90071-X 10.1103/PhysRevLett.92.120601 10.1216/RMJ-1974-4-3-407 10.1023/A:1010313423230 10.1088/0305-4470/17/2/023 10.1016/j.physa.2003.09.048 10.1103/PhysRevLett.53.419 10.1016/j.physrep.2008.12.001 |
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