Publications by authors named "CD Ball"

The current heightened social awareness and anxiety triggered by escalating violence against Black Americans in the United States demands a safe space for reflection, education, and civil discourse within the academic setting. Too often there is an unmet need paired with a collective urgent desire to better understand the chronic existing structural, social, educational, and health inequities affecting disadvantaged populations, particularly Black Americans. In this perspective, the authors provide insight into a shared learning approach that provided a forum to discuss Perspectives Against Racism (PAR).

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Raman spectral data collected with high-resolution laboratory spectrometers are processed into a format suitable for importing as a user library on a 1064 nm DeltaNu first generation, field-deployable spectrometer prototype. The two laboratory systems used are a 1064 nm Bruker Fourier transform (FT)-Raman spectrometer and a 785 nm Kaiser dispersive spectrometer. The steps taken to adapt for device-dependent spectral resolution, wavenumber shifts between instruments, and relative intensity response are described.

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Monte Carlo simulation is used to study binary mixtures of two-dimensional hard disks, confined to long, narrow, structureless pores with hard walls, in a regime of pore sizes where the large particles exhibit single file diffusion while the small particles diffuse normally. The dynamics of the small particles can be understood in the context of a hopping time, tau(21), that measures the time it takes for a small particle to escape the single file cage formed by its large particle neighbors, and can be linked to the long time diffusion coefficient. We find that tau(21) follows a power law as a function of the reduced pore radius for a wide range of particle size ratios with an exponent, alpha, that is independent of the size ratio, but linearly dependent on the Monte Carlo step size used in the dynamic scheme.

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A fairly strong molecular absorption band at 4429.27+/-0.04 Å, closely centered on the strongest diffuse interstellar band at 4428.

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