Evolution of perturbed accelerating relativistic shock waves (413 views) (PDF restricted 199 views)
Astrophys J Institute Of Physics Publishing (ISSN: 0004-637x), 2008 Oct 20; 686(2): 1103-1124.
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Paper type: Journal Article,
Impact factor: 6.331, 5-year impact factor: 5.743
Url: http://www.scopus.com/inward/record.url?eid=2-s2.0-54249132162&partnerID=40&md5=652327573ba90ac8976555ab1f5d7790
Keywords: Hydrodynamics, Shock Waves,
Affiliations:
*** IBB - CNR ***
Scuola Normale Superiore, Piazza dei Cavalieri 7, 56100 Pisa, Italy
Dipartimento di Fisica Generale Amedeo Avogadro, Università degli Studi di Torino, Via Pietro Giuria 1, 10125 Torino, Italy
INAF/Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy
Dipartimento di Astronomia e Scienza Dello Spazio, Università di Firenze, Largo Enrico Fermi 2, 50125 Firenze, Italy
References:
Not available.
Astrophys J Institute Of Physics Publishing (ISSN: 0004-637x), 2008 Oct 20; 686(2): 1103-1124.
Export to BibTeX Export to EndNote
Paper type: Journal Article,
Impact factor: 6.331, 5-year impact factor: 5.743
Url: http://www.scopus.com/inward/record.url?eid=2-s2.0-54249132162&partnerID=40&md5=652327573ba90ac8976555ab1f5d7790
Keywords: Hydrodynamics, Shock Waves,
Affiliations:
*** IBB - CNR ***
Scuola Normale Superiore, Piazza dei Cavalieri 7, 56100 Pisa, Italy
Dipartimento di Fisica Generale Amedeo Avogadro, Università degli Studi di Torino, Via Pietro Giuria 1, 10125 Torino, Italy
INAF/Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy
Dipartimento di Astronomia e Scienza Dello Spazio, Università di Firenze, Largo Enrico Fermi 2, 50125 Firenze, Italy
References:
Not available.
Evolution of perturbed accelerating relativistic shock waves
We study the evolution of an accelerating hyperrelativistic shock under the presence of upstream inhomogeneities wrinkling the discontinuity surface. The investigation is conducted by means of numerical simulations using the PLUTO code for astrophysical fluid dynamics. The reliability and robustness of the code are demonstrated against well-known results coming from the linear perturbation theory. We then follow the nonlinear evolution of two classes of perturbing upstream atmospheres and conclude that no lasting wrinkle can be preserved indefinitely by the flow. Finally, we derive analytically a description of the geometrical effects of a turbulent upstream ambient on the discontinuity surface. © 2008. The American Astronomical Society. All rights reserved.
We study the evolution of an accelerating hyperrelativistic shock under the presence of upstream inhomogeneities wrinkling the discontinuity surface. The investigation is conducted by means of numerical simulations using the PLUTO code for astrophysical fluid dynamics. The reliability and robustness of the code are demonstrated against well-known results coming from the linear perturbation theory. We then follow the nonlinear evolution of two classes of perturbing upstream atmospheres and conclude that no lasting wrinkle can be preserved indefinitely by the flow. Finally, we derive analytically a description of the geometrical effects of a turbulent upstream ambient on the discontinuity surface. © 2008. The American Astronomical Society. All rights reserved.
Evolution of perturbed accelerating relativistic shock waves
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Evolution of perturbed accelerating relativistic shock waves
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6 Records (6 excluding Abstracts).
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