Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics
In the initial stage of relativistic heavy-ion collisions, strong magnetic fields appear due to the large velocity of the colliding charges. The evolution of these fields appears as a novel and intriguing feature in the fluid-dynamical description of heavy-ion collisions. In this work, we study anal...
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doaj-ebccb2bcd1bd405c91df563795850c792020-11-25T01:04:40ZengElsevierPhysics Letters B0370-26931873-24452015-11-01750C455210.1016/j.physletb.2015.08.046Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamicsVictor Roy0Shi Pu1Luciano Rezzolla2Dirk Rischke3Institute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, 60438 Frankfurt am Main, GermanyInstitute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, 60438 Frankfurt am Main, GermanyInstitute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, 60438 Frankfurt am Main, GermanyInstitute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, 60438 Frankfurt am Main, GermanyIn the initial stage of relativistic heavy-ion collisions, strong magnetic fields appear due to the large velocity of the colliding charges. The evolution of these fields appears as a novel and intriguing feature in the fluid-dynamical description of heavy-ion collisions. In this work, we study analytically the one-dimensional, longitudinally boost-invariant motion of an ideal fluid in the presence of a transverse magnetic field. Interestingly, we find that, in the limit of ideal magnetohydrodynamics, i.e., for infinite conductivity, and irrespective of the strength of the initial magnetization, the decay of the fluid energy density e with proper time τ is the same as for the time-honoured “Bjorken flow” without magnetic field. Furthermore, when the magnetic field is assumed to decay ∼τ−a, where a is an arbitrary number, two classes of analytic solutions can be found depending on whether a is larger or smaller than one. In summary, the analytic solutions presented here highlight that the Bjorken flow is far more general than formerly thought. These solutions can serve both to gain insight on the dynamics of heavy-ion collisions in the presence of strong magnetic fields and as testbeds for numerical codes.http://www.sciencedirect.com/science/article/pii/S0370269315006474 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Victor Roy Shi Pu Luciano Rezzolla Dirk Rischke |
spellingShingle |
Victor Roy Shi Pu Luciano Rezzolla Dirk Rischke Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics Physics Letters B |
author_facet |
Victor Roy Shi Pu Luciano Rezzolla Dirk Rischke |
author_sort |
Victor Roy |
title |
Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics |
title_short |
Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics |
title_full |
Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics |
title_fullStr |
Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics |
title_full_unstemmed |
Analytic Bjorken flow in one-dimensional relativistic magnetohydrodynamics |
title_sort |
analytic bjorken flow in one-dimensional relativistic magnetohydrodynamics |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 1873-2445 |
publishDate |
2015-11-01 |
description |
In the initial stage of relativistic heavy-ion collisions, strong magnetic fields appear due to the large velocity of the colliding charges. The evolution of these fields appears as a novel and intriguing feature in the fluid-dynamical description of heavy-ion collisions. In this work, we study analytically the one-dimensional, longitudinally boost-invariant motion of an ideal fluid in the presence of a transverse magnetic field. Interestingly, we find that, in the limit of ideal magnetohydrodynamics, i.e., for infinite conductivity, and irrespective of the strength of the initial magnetization, the decay of the fluid energy density e with proper time τ is the same as for the time-honoured “Bjorken flow” without magnetic field. Furthermore, when the magnetic field is assumed to decay ∼τ−a, where a is an arbitrary number, two classes of analytic solutions can be found depending on whether a is larger or smaller than one. In summary, the analytic solutions presented here highlight that the Bjorken flow is far more general than formerly thought. These solutions can serve both to gain insight on the dynamics of heavy-ion collisions in the presence of strong magnetic fields and as testbeds for numerical codes. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269315006474 |
work_keys_str_mv |
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