Research & Reports

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Publications

 

Reports

Current Projects

The projects explored within WCAPP are varied. Below, we list the astrophysical problems, the suspected problem with atomic processes, and how to answer those problems.

A telescope image of the sun

Solar Opacity (SNL)

Problem: The solar convection zone boundary measured by helioseismology is discrepant with the standard solar model. This discrepancy can be resolved with a 14% increase in the Rosseland Mean Opacity.

Hypothesis: Opacity is incorrectly modeled.

Method: Heat a sample of iron to solar interior conditions to measure opacity in absorption (see Bailey et al. 2015).

 

 

A telescope image of a white dwarf

White Dwarf Spectral Line-Broadening (UT)

Problem: Spectroscopic method of determining white dwarf masses is discrepant with gravitational redshift and orbital determination of mass.

Hypothesis: Spectral Line Broadening is inaccurate.

Method: Heat samples of hydrogen and helium gasses to white dwarf atmospheric conditions and measure emission and absorption spectra and compare to models (see Montgomery et al. 2015.

 

A telescope image of a black object emitting blue light

Efficiency of RAD (SNL)

Problem: Is Resonant Auger Destruction (RAD) the explanation for missing iron lines in accretion disks?

Hypothesis: RAD is not 100% efficient in destroying emission lines

Method: Heat sample of silicon in high-radiation environment, measure spectrum in emission and absorption to measure relative strengths of spectral lines and how they are affected by RAD (see Loisel et al. 2017).

 

A telescope image of a bright object surrounded by brown disks

Heating in Accretion Disks (UNR)

Problem: Accretion disk models rely on untested atomic kinetics models.

Hypothesis: The current models (XSTAR, CLOUDY) are not accurately capturing atomic kinetics properly.

Method: Heat neon to accretion disk conditions and compare charge-states and line strengths with the predictions of astrophysical codes (Mancini et al. 2017). 

 

Publications

2024
2023
2022
2021
2020 & prior

Reports

National Nuclear Security Administration (NNSA)

Research Performance Progress Reports (RPPR) are management reports which provide information on project status, and are submitted to NNSA 90 days after end of each budget period.

Year 3 - RPPR 2021 

Year 2 - RPPR 2020

Year 1 - RPPR 2019 

Center Scientific Advisory Committee (CSAC)

The CSAC is an external advisory and review board for the Center that continually strengthens the Center and its contributions to meeting the goals of the SSAA Program. The CSAC meets at the Center annually to review progress and scientific plans, and to advise on management of the Center and on planning for future collaboration.  The CSAC then produces an annual report of Findings and Recommendations from the review and submits to the Center director and SSAP.

Year 4 - CSAC Report, 2022

Year 3 - CSAC Report, 2021

Year 2 - CSAC Report, 2020

Year 1 - CSAC Report, 2019