How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants

C. C. Kuranz, H.-S. Park, C. M. Huntington, A. R. Miles, B. A. Remington, T. Plewa, M. R. Trantham, H. F. Robey, D. Shvarts, A. Shimony, K. Raman, S. MacLaren, W. C. Wan, F. W. Doss, J. Kline, K. A. Flippo, G. Malamud, T. A. Handy, S. Prisbrey, C. M. Krauland, S. R. Klein, E. C. Harding, R. Wallace, M. J. Grosskopf, D. C. Marion, D. Kalantar, E. Giraldez, R. P. Drake

Open source

DOI: 10.1038/s41467-018-03548-7
Published: 2018-04-19
Container: Nature Communications
Publisher: Springer Science and Business Media LLC
Open access: unknown

Credibility signals

uncertain Score 64/100 under policy 1.0.0. This is a metadata assessment, not a judgment of the paper's conclusions.

Show all credibility signals

supportingDOI registered: A matching record was returned by Crossref. Source: Crossref; license: CC0 metadata
supportingDOI resolves: A matching record was returned by Crossref. Source: Crossref; license: CC0 metadata
not scoredDirectory of Open Access Journals: No matching DOAJ record was present in this response. No allow-list match; this is not evidence of low credibility. Source: DOAJ; license: CC0
not scoredMEDLINE indexed: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredOpenAlex core source: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredKnown publisher allow-list: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredROR affiliation: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredRetraction Watch retraction: No retraction notice matched this DOI in the deployed snapshot. No matching event found; coverage may be incomplete. Source: Retraction Watch; license: CC BY 4.0
not scoredRetraction Watch expression of concern: No expression of concern notice matched this DOI in the deployed snapshot. No matching event found; coverage may be incomplete. Source: Retraction Watch; license: CC BY 4.0
not scoredRetraction Watch correction: No correction notice matched this DOI in the deployed snapshot. No matching event found; coverage may be incomplete. Source: Retraction Watch; license: CC BY 4.0
not scoredRetraction Watch reinstatement: No reinstatement notice matched this DOI in the deployed snapshot. No matching event found; coverage may be incomplete. Source: Retraction Watch; license: CC BY 4.0
not scoredOpen access status: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredPublication license: Not checked or no result supplied; no credibility inference made. Source: No authority result supplied; license: Unknown
not scoredPublication version: A publication version was supplied but is not scored. Source: Normalized work metadata; license: Caller-provided; provenance license not supplied to scorer
supportingMetadata completeness: All 6 scored descriptive metadata groups are present. Source: Normalized work metadata; license: Caller-provided; provenance license not supplied to scorer

Cite this work

BibTeX

@article{allodium:10.1038/s41467-018-03548-7,
  title = {How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants},
  author = {C. C. Kuranz and H.-S. Park and C. M. Huntington and A. R. Miles and B. A. Remington and T. Plewa and M. R. Trantham and H. F. Robey and D. Shvarts and A. Shimony and K. Raman and S. MacLaren and W. C. Wan and F. W. Doss and J. Kline and K. A. Flippo and G. Malamud and T. A. Handy and S. Prisbrey and C. M. Krauland and S. R. Klein and E. C. Harding and R. Wallace and M. J. Grosskopf and D. C. Marion and D. Kalantar and E. Giraldez and R. P. Drake},
  year = {2018},
  journal = {Nature Communications},
  doi = {10.1038/s41467-018-03548-7},
  url = {https://doi.org/10.1038/s41467-018-03548-7}
}

RIS

TY  - JOUR
TI  - How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
AU  - C. C. Kuranz
AU  - H.-S. Park
AU  - C. M. Huntington
AU  - A. R. Miles
AU  - B. A. Remington
AU  - T. Plewa
AU  - M. R. Trantham
AU  - H. F. Robey
AU  - D. Shvarts
AU  - A. Shimony
AU  - K. Raman
AU  - S. MacLaren
AU  - W. C. Wan
AU  - F. W. Doss
AU  - J. Kline
AU  - K. A. Flippo
AU  - G. Malamud
AU  - T. A. Handy
AU  - S. Prisbrey
AU  - C. M. Krauland
AU  - S. R. Klein
AU  - E. C. Harding
AU  - R. Wallace
AU  - M. J. Grosskopf
AU  - D. C. Marion
AU  - D. Kalantar
AU  - E. Giraldez
AU  - R. P. Drake
PY  - 2018
JO  - Nature Communications
DO  - 10.1038/s41467-018-03548-7
UR  - https://doi.org/10.1038/s41467-018-03548-7
ER  -

APA

Kuranz, C. C., Park, H., Huntington, C. M., Miles, A. R., Remington, B. A., Plewa, T., Trantham, M. R., Robey, H. F., Shvarts, D., Shimony, A., Raman, K., MacLaren, S., Wan, W. C., Doss, F. W., Kline, J., Flippo, K. A., Malamud, G., Handy, T. A., Prisbrey, S., Krauland, C. M., Klein, S. R., Harding, E. C., Wallace, R., Grosskopf, M. J., Marion, D. C., Kalantar, D., Giraldez, E., & Drake, R. P. (2018). How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants. Nature Communications. https://doi.org/10.1038/s41467-018-03548-7

Source records

crossref · retrieved 2026-11-07T08:44:06.542Z