Evidence map›Paper›PMID 37862409›Full record

ArticleScience advances2023

Ultrafast x-ray detection of low-spin iron in molten silicate under deep planetary interior conditions.

Sang-Heon Shim, Byeongkwan Ko, Dimosthenis Sokaras, Bob Nagler, He Ja Lee, Eric Galtier, Siegfried Glenzer, Eduardo Granados, Tommaso Vinci, Guillaume Fiquet and 8 more

Open access · goldAbstract read
In one paragraph

Article in Science advances, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 3 papers.

0numbers the graph read from it
0cells of the map it votes in
3citing papers in PubMed
2.0field-weighted citation impact, top 15% of its field
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

3 citing papers in PubMed, 7 citations in OpenAlex.

  1. Article
  2. Electrical and thermal conductivity of Earth's iron-enriched basal magma ocean.Proceedings of the National Academy of Sciences of the United States of America · 2025
    Article
  3. Review
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

18 authors at 4 institutions in 2 countries.

Sang-Heon ShimSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.ORCID 0000-0001-5203-6038
Byeongkwan KoSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
Dimosthenis SokarasSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0001-8117-1933
Bob NaglerSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0009-0002-5736-7842
He Ja LeeSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0002-4035-5637
Eric GaltierSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0002-0396-285X
Siegfried GlenzerSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0001-9112-0558
Eduardo GranadosSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.
Tommaso VinciLaboratoire pour l'Utilisation des Lasers Intenses (LULI), Ecole Polytechnique, CNRS, CEA, UPMC, 91128 Palaiseau, France.ORCID 0000-0002-1595-1752
Guillaume FiquetSorbonne Université, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, Museum National d'Histoire Naturelle, UMR CNRS 7590, 4 Place Jussieu, 75005 Paris, France.ORCID 0000-0001-8961-3281
Jonathan DolinschiSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.ORCID 0000-0002-6926-2645
Jackie TappanSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
Britany KulkaSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.ORCID 0000-0001-7873-5267
Wendy L MaoSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0003-0595-7760
Guillaume MorardSorbonne Université, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, Museum National d'Histoire Naturelle, UMR CNRS 7590, 4 Place Jussieu, 75005 Paris, France.ORCID 0000-0002-4225-0767
Alessandra RavasioLaboratoire pour l'Utilisation des Lasers Intenses (LULI), Ecole Polytechnique, CNRS, CEA, UPMC, 91128 Palaiseau, France.ORCID 0000-0002-2077-6493
Arianna GleasonSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0002-7736-5118
Roberto Alonso-MoriSLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA.ORCID 0000-0002-5357-0934
SLAC National Accelerator Laboratory · USArizona State University · USCentre National de la Recherche Scientifique · FRPlanetary Science Institute · US

Funding

Structural Dynamics at LCLSP41GM139687 · NIGMS · STANFORD UNIVERSITY · PI HUNTER, MARK · 2021 to 2025
$7.5M
NIGMS NIH HHS P41 GM139687
6 · The paper itself

Abstract

The spin state of Fe can alter the key physical properties of silicate melts, affecting the early differentiation and the dynamic stability of the melts in the deep rocky planets. The low-spin state of Fe can increase the affinity of Fe for the melt over the solid phases and the electrical conductivity of melt at high pressures. However, the spin state of Fe has never been measured in dense silicate melts due to experimental challenges. We report detection of dominantly low-spin Fe in dynamically compressed olivine melt at 150 to 256 gigapascals and 3000 to 6000 kelvin using laser-driven shock wave compression combined with femtosecond x-ray diffraction and x-ray emission spectroscopy using an x-ray free electron laser. The observation of dominantly low-spin Fe supports gravitationally stable melt in the deep mantle and generation of a dynamo from the silicate melt portion of rocky planets.

Identifiers

PMID37862409
PMCPMC10588943
OpenAlexW4387823508

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.