Research & Reports

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).