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Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities: A modeling tool for astrophysics

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Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities : A modeling tool for astrophysics. / Oks, E.; Dalimier, E.; Faenov, A. Ya; Angelo, P.; Pikuz, S. A.; Tubman, E.; Butler, N. M H; Dance, R. J.; Pikuz, T. A.; Skobelev, I. Yu; Alkhimova, M. A.; Booth, N.; Green, J.; Gregory, C.; Andreev, A.; Zhidkov, A.; Kodama, R.; McKenna, P.; Woolsey, N.

In: Optics Express, Vol. 25, No. 3, 06.02.2017, p. 1958-1972.

Research output: Contribution to journalArticle

Harvard

Oks, E, Dalimier, E, Faenov, AY, Angelo, P, Pikuz, SA, Tubman, E, Butler, NMH, Dance, RJ, Pikuz, TA, Skobelev, IY, Alkhimova, MA, Booth, N, Green, J, Gregory, C, Andreev, A, Zhidkov, A, Kodama, R, McKenna, P & Woolsey, N 2017, 'Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities: A modeling tool for astrophysics', Optics Express, vol. 25, no. 3, pp. 1958-1972. https://doi.org/10.1364/OE.25.001958

APA

Oks, E., Dalimier, E., Faenov, A. Y., Angelo, P., Pikuz, S. A., Tubman, E., ... Woolsey, N. (2017). Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities: A modeling tool for astrophysics. Optics Express, 25(3), 1958-1972. https://doi.org/10.1364/OE.25.001958

Vancouver

Oks E, Dalimier E, Faenov AY, Angelo P, Pikuz SA, Tubman E et al. Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities: A modeling tool for astrophysics. Optics Express. 2017 Feb 6;25(3):1958-1972. https://doi.org/10.1364/OE.25.001958

Author

Oks, E. ; Dalimier, E. ; Faenov, A. Ya ; Angelo, P. ; Pikuz, S. A. ; Tubman, E. ; Butler, N. M H ; Dance, R. J. ; Pikuz, T. A. ; Skobelev, I. Yu ; Alkhimova, M. A. ; Booth, N. ; Green, J. ; Gregory, C. ; Andreev, A. ; Zhidkov, A. ; Kodama, R. ; McKenna, P. ; Woolsey, N. / Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities : A modeling tool for astrophysics. In: Optics Express. 2017 ; Vol. 25, No. 3. pp. 1958-1972.

Bibtex - Download

@article{d2ab45f4e9b3418384dbe32907d968c1,
title = "Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities: A modeling tool for astrophysics",
abstract = "By analyzing profiles of experimental x-ray spectral lines of Si XIV and Al XIII, we found that both Langmuir and ion acoustic waves developed in plasmas produced via irradiation of thin Si foils by relativistic laser pulses (intensities ∼1021 W/cm2). We prove that these waves are due to the parametric decay instability (PDI). This is the first time that the PDI-induced ion acoustic turbulence was discovered by the x-ray spectroscopy in laser-produced plasmas. These conclusions are also supported by PIC simulations. Our results can be used for laboratory modeling of physical processes in astrophysical objects and a better understanding of intense laser-plasma interactions.",
author = "E. Oks and E. Dalimier and Faenov, {A. Ya} and P. Angelo and Pikuz, {S. A.} and E. Tubman and Butler, {N. M H} and Dance, {R. J.} and Pikuz, {T. A.} and Skobelev, {I. Yu} and Alkhimova, {M. A.} and N. Booth and J. Green and C. Gregory and A. Andreev and A. Zhidkov and R. Kodama and P. McKenna and N. Woolsey",
note = "{\circledC} 2017 Optical Society of America. This is an author-produced version of the published paper. Uploaded in accordance with the publisher’s self-archiving policy. Further copying may not be permitted; contact the publisher for details.",
year = "2017",
month = "2",
day = "6",
doi = "10.1364/OE.25.001958",
language = "English",
volume = "25",
pages = "1958--1972",
journal = "Optics Express",
issn = "1094-4087",
publisher = "The Optical Society",
number = "3",

}

RIS (suitable for import to EndNote) - Download

TY - JOUR

T1 - Using X-ray spectroscopy of relativistic laser plasma interaction to reveal parametric decay instabilities

T2 - A modeling tool for astrophysics

AU - Oks, E.

AU - Dalimier, E.

AU - Faenov, A. Ya

AU - Angelo, P.

AU - Pikuz, S. A.

AU - Tubman, E.

AU - Butler, N. M H

AU - Dance, R. J.

AU - Pikuz, T. A.

AU - Skobelev, I. Yu

AU - Alkhimova, M. A.

AU - Booth, N.

AU - Green, J.

AU - Gregory, C.

AU - Andreev, A.

AU - Zhidkov, A.

AU - Kodama, R.

AU - McKenna, P.

AU - Woolsey, N.

N1 - © 2017 Optical Society of America. This is an author-produced version of the published paper. Uploaded in accordance with the publisher’s self-archiving policy. Further copying may not be permitted; contact the publisher for details.

PY - 2017/2/6

Y1 - 2017/2/6

N2 - By analyzing profiles of experimental x-ray spectral lines of Si XIV and Al XIII, we found that both Langmuir and ion acoustic waves developed in plasmas produced via irradiation of thin Si foils by relativistic laser pulses (intensities ∼1021 W/cm2). We prove that these waves are due to the parametric decay instability (PDI). This is the first time that the PDI-induced ion acoustic turbulence was discovered by the x-ray spectroscopy in laser-produced plasmas. These conclusions are also supported by PIC simulations. Our results can be used for laboratory modeling of physical processes in astrophysical objects and a better understanding of intense laser-plasma interactions.

AB - By analyzing profiles of experimental x-ray spectral lines of Si XIV and Al XIII, we found that both Langmuir and ion acoustic waves developed in plasmas produced via irradiation of thin Si foils by relativistic laser pulses (intensities ∼1021 W/cm2). We prove that these waves are due to the parametric decay instability (PDI). This is the first time that the PDI-induced ion acoustic turbulence was discovered by the x-ray spectroscopy in laser-produced plasmas. These conclusions are also supported by PIC simulations. Our results can be used for laboratory modeling of physical processes in astrophysical objects and a better understanding of intense laser-plasma interactions.

UR - http://www.scopus.com/inward/record.url?scp=85011702113&partnerID=8YFLogxK

U2 - 10.1364/OE.25.001958

DO - 10.1364/OE.25.001958

M3 - Article

VL - 25

SP - 1958

EP - 1972

JO - Optics Express

JF - Optics Express

SN - 1094-4087

IS - 3

ER -