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Daiki Takama

Publications and source records attributed to Daiki Takama.

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Measurement of the Temperature Dependence of the Refractive Index of CdZnTe

We have been developing a CdZnTe immersion grating for a compact high-dispersion mid-infrared spectrometer (wavelength range 10--18 $μ$m, spectral resolution $R = λ/Δλ> 25,000$, operating temperature $T < 20$ K). Using an immersion grating, the spectrometer size can be reduced to $1/n$ ($n$: refractive index) compared to conventional diffraction gratings. CdZnTe is promising as a material for immersion gratings for the wavelength range. However, the refractive index $n$ of CdZnTe has not been measured at $T < 20$ K. We have been developing a system to precisely measure $n$ at cryogenic temperatures ($T \sim 10$ K) in the mid-infrared wavelength range. As the first result, this paper reports the temperature dependence of $n$ of CdZnTe at the wavelength of 10.68 $μ$m. This system employs the minimum deviation method. The refractive index $n$ of CdZnTe is measured at temperatures of \( T = 12.57, 22.47, 50.59, 70.57, \text{ and } 298 \, \text{K} \). We find that $n$ of CdZnTe at $λ=$ 10.68 $μ$m is $2.6371 \pm 0.0022$ at $12.57 \pm 0.14$ K, and the average temperature dependence of $n$ between 12.57 $\pm$ 0.14 K and 70.57 $\pm$ 0.23 K is $Δn/ΔT = (5.8 \pm 0.3) \times 10^{-5}$ K$^{-1}$.

astro-ph.IM

Mid-Infrared Imaging Spectroscopy of N2O Solid Simulating the haze of trans-Neptunian objects

\ Nitrous oxide (N$_2$O) ice is likely to exist in trans-Neptunian objects such as Pluto and Triton, potentially formed through ultraviolet (UV) radiation from the Sun or cosmic ray irradiation of N$_2$ and CO ices. However, the mid-infrared spectral characteristics of N$_2$O ice in higher temperature regions (90-110 K), changes in mid-infrared spectra during UV irradiation, and the chemical network of nitrogen oxide (N$_x$O$_y$) ices remain insufficiently understood. This study aims to elucidate these aspects through in-situ mid-infrared spectral measurements of cryogenic particles using two-dimensional imaging Fourier transform infrared spectroscopy. Spectroscopic imaging confirmed strong absorption at 7.75 $μ$m (N$_2$O $ν_1$ vibrational mode), with weaker vibrational modes observed at 8.60 $μ$m (N$_2$O 2$ν_2$), 7.27 $μ$m (N$_2$O torsion), and 5.29 $μ$m (N$_2$O $ν_1$+$ν_2$). Annealing experiments simulating high-temperature conditions demonstrated that all vibrational modes irreversibly intensified with increasing temperature, indicating progressive crystallization. New spectral features appeared at approximately 12 $μ$m and 14 $μ$m at the condensed sample. N$_2$O ice was exposed to ultraviolet radiation (190-340 nm) using a D$_2$ lamp for 8.5 hours to investigate spectral changes during UV irradiation. After 60-90 minutes of irradiation, all N$_2$O vibrational modes disappeared, while absorption intensities of various nitrogen oxides, including NO, NO$_2$, N$_2$O$_3$, and O$_3$ increased. Beyond 180 minutes, vibrational modes of multiple nitrogen oxide ices exhibited intensity variations across different wavelengths, corresponding to other species such as cis-(NO)$_2$, N$_2$O$_4$, and N$_2$O$_5$.

astro-ph.EP