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A higher-than-predicted measurement of iron opacity at solar interior temperatures

Author

Listed:
  • J. E. Bailey

    (Sandia National Laboratories, 1515 Eubank SE)

  • T. Nagayama

    (Sandia National Laboratories, 1515 Eubank SE)

  • G. P. Loisel

    (Sandia National Laboratories, 1515 Eubank SE)

  • G. A. Rochau

    (Sandia National Laboratories, 1515 Eubank SE)

  • C. Blancard

    (Commissariat à l’Énergie Atomique (CEA) et aux Énergies Alternatives, F-91297 Arpajon, France)

  • J. Colgan

    (Los Alamos National Laboratory, Bikini Atoll Road)

  • Ph. Cosse

    (Commissariat à l’Énergie Atomique (CEA) et aux Énergies Alternatives, F-91297 Arpajon, France)

  • G. Faussurier

    (Commissariat à l’Énergie Atomique (CEA) et aux Énergies Alternatives, F-91297 Arpajon, France)

  • C. J. Fontes

    (Los Alamos National Laboratory, Bikini Atoll Road)

  • F. Gilleron

    (Commissariat à l’Énergie Atomique (CEA) et aux Énergies Alternatives, F-91297 Arpajon, France)

  • I. Golovkin

    (Prism Computational Sciences, 455 Science Drive, Suite 140, Madison, Wisconsin 53711, USA)

  • S. B. Hansen

    (Sandia National Laboratories, 1515 Eubank SE)

  • C. A. Iglesias

    (Lawrence Livermore National Laboratory, 7000 East Avenue)

  • D. P. Kilcrease

    (Los Alamos National Laboratory, Bikini Atoll Road)

  • J. J. MacFarlane

    (Prism Computational Sciences, 455 Science Drive, Suite 140, Madison, Wisconsin 53711, USA)

  • R. C. Mancini

    (University of Nevada, 1664 North Virginia Street)

  • S. N. Nahar

    (Ohio State University, 140 West 18th Avenue)

  • C. Orban

    (Ohio State University, 140 West 18th Avenue)

  • J.-C. Pain

    (Commissariat à l’Énergie Atomique (CEA) et aux Énergies Alternatives, F-91297 Arpajon, France)

  • A. K. Pradhan

    (Ohio State University, 140 West 18th Avenue)

  • M. Sherrill

    (Los Alamos National Laboratory, Bikini Atoll Road)

  • B. G. Wilson

    (Lawrence Livermore National Laboratory, 7000 East Avenue)

Abstract

Laboratory measurements of iron opacity made under conditions similar to those inside the Sun reveal much higher opacity than predicted, helping to resolve inconsistencies within stellar models of the internal temperatures of stars.

Suggested Citation

  • J. E. Bailey & T. Nagayama & G. P. Loisel & G. A. Rochau & C. Blancard & J. Colgan & Ph. Cosse & G. Faussurier & C. J. Fontes & F. Gilleron & I. Golovkin & S. B. Hansen & C. A. Iglesias & D. P. Kilcre, 2015. "A higher-than-predicted measurement of iron opacity at solar interior temperatures," Nature, Nature, vol. 517(7532), pages 56-59, January.
    • Handle: RePEc:nat:nature:v:517:y:2015:i:7532:d:10.1038_nature14048
    DOI: 10.1038/nature14048
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    Cited by:

    1. Ryan Babbush & William J. Huggins & Dominic W. Berry & Shu Fay Ung & Andrew Zhao & David R. Reichman & Hartmut Neven & Andrew D. Baczewski & Joonho Lee, 2023. "Quantum simulation of exact electron dynamics can be more efficient than classical mean-field methods," Nature Communications, Nature, vol. 14(1), pages 1-9, December.
    2. Tobias Dornheim & Maximilian Böhme & Dominik Kraus & Tilo Döppner & Thomas R. Preston & Zhandos A. Moldabekov & Jan Vorberger, 2022. "Accurate temperature diagnostics for matter under extreme conditions," Nature Communications, Nature, vol. 13(1), pages 1-7, December.
    3. S. X. Hu & David T. Bishel & David A. Chin & Philip M. Nilson & Valentin V. Karasiev & Igor E. Golovkin & Ming Gu & Stephanie B. Hansen & Deyan I. Mihaylov & Nathaniel R. Shaffer & Shuai Zhang & Timot, 2022. "Probing atomic physics at ultrahigh pressure using laser-driven implosions," Nature Communications, Nature, vol. 13(1), pages 1-11, December.

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