A nonthermal carbon monoxide plasma is known to produce a solid deposition which is thought to be a polymer of carbon suboxide (C3O2); however there are very few investigations of this deposition in the literature. This thesis contains an analysis of the theoretical thermodynamics and kinetics of carbon suboxide formation as well as experimental results. The theoretical analysis suggests that carbon suboxide may be an equilibrium product even at ambient conditions but favors lower temperatures; furthermore if solid carbon is considered to be kinetically limited, and therefore not a product, then carbon suboxide is more likely to be a product under these pseudo-equilibrium conditions. Experimentally, solid films were produced in a dielectric barrier discharge (DBD) containing pure carbon monoxide. Optical emission spectroscopy was used to analyze the plasma and models of the emission spectra were created to determine the plasma temperatures. Deposition rates were determined to be on the order of 0.2 mg/min at a power of about 10W; it is expected however that these conditions are not optimized. The overall kinetics of carbon suboxide was analyzed and optimal conditions for operation can be estimated. Characterization of the solid depositions were carried out using Solid State Nuclear Magnetic Resonance (NMR), Fourier Transform Infrared Spectroscopy (FTIR), Electrospray Ionization Mass Spectroscopy (ESI-MS), and Matrix-assisted Laser Desorption Ionization Mass Spectroscopy (MALDI-MS). The characteristics of the film are very comparable to hydrolyzed carbon suboxide polymer suggesting that carbon suboxide polymer were in fact created in the carbon monoxide plasma at atmospheric conditions.

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Supernovae (SNe) are energetic explosions that signal the end of a star's life. These events and the supernova remnants (SNRs) they leave behind play a central role in stellar feedback by adding energy and momentum and metals to the interstellar medium (ISM). Emission associated with these feedback processes, especially atomic and molecular line emission as well as thermal and nonthermal continuum emission is known to be enhanced in regions of high density, such as dense circumstellar matter (CSM) around SNe and molecular clouds (MCs). In this thesis, I begin with a brief overview of the physics of SN shocks in Chapter 1, focusing on a foundation for studying pan-chromatic signatures of interactions between SNe and dense environments. In Chapter 2, I examine an unusual SN with signatures of CSM interaction in the form of narrow lines of hydrogen (Type IIn) and thermal continuum emission. This SN appears to belong to a class of Type Ia SNe that shares spectroscopic features with Type IIn SNe. I discuss the difficulties of decomposing spectra in a regime where interaction occurs between SN ejecta and CSM, potentially confusing the underlying SN type. This is followed by a discussion of rebrightening that occurred at late-time in 𝐵 and 𝑉 band photometry of this SN, possibly associated with clumpy or dense CSM at large distances from the progenitor. In Chapter 3, I examine synchrotron emission from Cassiopeia A, observed in the 𝐾ₛ band over multiple epochs. The synchrotron emission is generally diffuse over the remnant, but there is one location in the southwest portion of the remnant where it appears to be enhanced and entrained as knots of emission in the SNR ejecta. I evaluate whether the 𝐾ₛ band knots are dominated by synchrotron emission by comparing them to other infrared and radio imaging that is known to be dominated by synchrotron emission. Concluding that they are likely synchrotron-emitting knots, I measure the magnetic field strength and electron density required for their evolution over the ~ 10 yr baseline they were observed and find 𝐵 ≈ 1.3-5.8 mG and 𝑛ₑ≈ 1,000-15,000 cm⁻³. The magnetic field strengths appear enhanced beyond values required by the adiabatic strong shock limit, arguing in favor of other forms of magnetic field amplification in the shock. In Chapter 4, I again discuss Cassiopeia A and interaction between the remnant and nearby MCs as seen at mid-infrared and millimeter wavelengths. I report detection of a SNR-MC interaction and analyze its signatures in broadened molecular lines. I extend this analysis in Chapter 5 to a large survey for SNR-MC interactions in the ¹²CO 𝐽=2-1 line. Although broadened ¹²CO 𝐽=2-1 line emission should be detectable toward virtually all SNR-MC interactions, I find relatively few examples; therefore, the number of interactions is low. This result favors mechanisms other than supernova feedback as the basic trigger for star formation. In addition, I find no significant association between TeV gamma-ray sources and MC interactions, contrary to predictions that SNR-MC interfaces are the primary venues for cosmic ray acceleration. I end this dissertation in Chapter 6 with a brief summary of my results and two extensions of this work: examining the late-time radio light curves of CSM-interacting SNe for signatures of radio synchrotron emission and dense or clumpy CSM at large distances from the progenitor and re-observing SNR-MC interactions in ¹²CO 𝐽=3-2 in order to verify the presence of shock-heated molecular gas and perform a census on the densities and temperatures of post-shock molecular gas.

In this study conducted at Food Science Australia (FSA) and Berlin University of Technology (BUT), the effects of pulsed electric field (PEF) treatment, a novel non-thermal processing technology on bovine milk microflora and native enzymes and on the rheological and textural properties of rennet-induced milk gels was investigated. The PEF treatments were conducted at field intensities of 25-37 kV cm-1 (up to 50 kV cm-1)and temperature range of 30°C to 75ºC. Native milk enzymes selected for the study included alkaline phosphatase, lipase, xanthine oxidase and plasminand microbiological study included determining Total Plate Count (TPC) and Pseudomonas and Enterobacteriaceae counts in skim milk. At 30ºC PEF treatment at maximum field intensity inactivated AlP by 42% while at 60oC inactivation was higher (67%). Under these treatment conditions less than1 log reduction in TPC and Pseudomonas count and 2.1 logs reduction in the Enterobacteriaceae count was achieved at 30oC while at 60ºC TPC dropped by 2.4 logs and Pseudomonas and Enterobacteriaceae counts were reduced by 5.9 and 2.1 logs, respectively to below the detection limit of 1 CFU mL-1. Combining PEF treatment with heat increased the inactivation level of all enzymes which showed an increasing trend with increasing field intensity and temperature. Treatment time (4.8, 9.6, 19.2, 28.8 and 38.4 µs) was controlled by either changing the pulse frequencies (100-400 Hz) or product flow rate (30-240 mL min-1) at a constant field intensity of 31 kV cm-1 and it was found that changing the flow rate was a more effective way of enzyme inactivation than changing the frequency due to longer exposure time of enzymes to heat and field intensity. The size of casein micelles and fat globules was not affected by PEF treatment while severe heating of milk at 97oC for 10 min decreased both micelle and fat globule sizes marginally. The coagulation time of rennet-induced gels made from PEF-treated (35 to 50 kV cm-1) milks (whole and skim) increased as the treatment intensity increased, but remained shorter than gels made from pasteurised milk. The PEF treatment of milk at various field intensities and temperatures adversely affected the G′, G′′ and firmness of gels, but the effects were less pronounced than in gels made from pasteurised milks. This study concludes that for successful application in milk processing the PEF treatment needs to be combined with mild heat treatment. This approach could achieve safer milk with less damage to milk functionality. However, the quest for a suitable quality assurance indicator enzyme will need more extensive studies.

The PEF treatments were conducted at field intensities of 25-37 kV cm-1 (up to 50 kV cm-1)and temperature range of 30°C to 75ºC. Native milk enzymes selected for the study included alkaline phosphatase, lipase, xanthine oxidase and plasminand microbiological study included determining Total Plate Count (TPC) and Pseudomonas and Enterobacteriaceae counts in skim milk. At 30ºC PEF treatment at maximum field intensity inactivated AlP by 42% while at 60oC inactivation was higher (67%). Under these treatment conditions less than1 log reduction in TPC and Pseudomonas count and 2.1 logs reduction in the Enterobacteriaceae count was achieved at 30oC while at 60ºC TPC dropped by 2.4 logs and Pseudomonas and Enterobacteriaceae counts were reduced by 5.9 and 2.1 logs, respectively to below the detection limit of 1 CFU mL-1. Combining PEF treatment with heat increased the inactivation level of all enzymes which showed an increasing trend with increasing field intensity and temperature. Treatment time (4.8, 9.6, 19.2, 28.8 and 38.4 µs) was controlled by either changing the pulse frequencies (100-400 Hz) or product flow rate (30-240 mL min-1) at a constant field intensity of 31 kV cm-1 and it was found that changing the flow rate was a more effective way of enzyme inactivation than changing the frequency due to longer exposure time of enzymes to heat and field intensity. The size of casein micelles and fat globules was not affected by PEF treatment while severe heating of milk at 97oC for 10 min decreased both micelle and fat globule sizes marginally. The coagulation time of rennet-induced gels made from PEF-treated (35 to 50 kV cm-1) milks (whole and skim) increased as the treatment intensity increased, but remained shorter than gels made from pasteurised milk. The PEF treatment of milk at various field intensities and temperatures adversely affected the G′, G′′ and firmness of gels, but the effects were less pronounced than in gels made from pasteurised milks. This study concludes that for successful application in milk processing the PEF treatment needs to be combined with mild heat treatment. This approach could achieve safer milk with less damage to milk functionality. However, the quest for a suitable quality assurance indicator enzyme will need more extensive studies.

Milk is one of the eight major food allergens. Cow's milk allergy is the most common allergy in children under 2 years of age. About 1.6 to 2.8 percent of children under this age are reported to have cow's milk allergy. Casein, β-lactoglobulin and α-lactalbumin are major milk protein allergens. Nonthermal treatments like high intensity ultrasound, ultraviolet (UV) light and nonthermal plasma treatments have been reported in the literature to be effective in reducing the allergenicity of different food proteins. Hence it was expected for these treatments to reduce cow milk allergenicity. The objective of this study was to investigate the effect of high intensity ultrasound, nonthermal atmospheric plasma and UV-C light treatments in reducing the allergenicity of isolated major milk proteins. Sonics Vibracell VC 505 ultrasonic liquid processor was used to perform high intensity ultrasound treatments. UV light treatments were performed using a DDK Scientific Corporation UV tunnel. A nonthermal atmospheric plasma setup assembled in Department of Microbiology lab was used to perform plasma treatments. Samples were analyzed using sodium dodecyl sulfate-polyacrylamide gel electrophoresis (SDS-PAGE) to estimate the change in protein concentration and enzyme linked immuno sorbent assays (ELISA) to observe the change in IgE binding. A one-way analysis of variance was conducted to evaluate the relationship between treatment time and percent IgE binding at 95% confidence level. Further investigation was conducted with nuclear magnetic resonance (NMR) spectroscopy on treated casein to assess any change in the structure of protein. SDS-PAGE results for ultrasound and plasma treatments didn't show any change in gel band intensities for casein, β-lactoglobulin and α-lactalbumin indicating no significant change in protein concentration. Ci-ELISA analysis showed that there was no significant difference (p>0.05) in IgE binding values for control and treated samples in ultrasound and plasma treatment conditions tested in this study. The intensities of all the three protein bands in SDS-PAGE gel were reduced by UV-C light treatment at 15 min treatment time. In Ci-ELISA, there was a significant difference (p< 0.05) in IgE binding values for control and treated samples and a reduction in allergenicity of proteins (25% reduction for casein and 28% reduction for whey protein fractions) was observed. Further investigations using in vivo clinical trials need to be conducted to confirm this result. NMR results didn't show any noticeable changes in the structures of casein with all three different treatments. In conclusion, UV-C light treatment can reduce the allergenicity of isolated major milk proteins to some extent. High intensity ultrasound and nonthermal atmospheric plasma treatments failed to generate effective results for reducing allergenicity at the conditions tested in this study. Higher intensity and longer treatment conditions might yield better results with ultrasound treatment. Different power and gas flow rates used to generate plasma with direct exposure of proteins might yield better results towards reducing the allergenicity of major milk allergens.

The natural water inside green coconuts is regarded as a healthy drink due to the elements of nutritional and therapeutic value. Since there is chance of contamination of tender coconut water (TCW) with psychrophilic microbes during extraction from its hard shell if stored at 4 ºC, thermal pasteurization is currently practiced. However, the thermal treatment of TCW causes a rise in off flavors and loss of the vital nutrients. To solve this problem, a non-thermal pasteurization technology is desirable. The goal of this research was to assess the antimicrobial effectiveness of ultraviolet light C (UVC) as non-thermal pasteurization of TCW and evaluation of physico-chemical and sensory quality of the treated TCW in comparison to the fresh TCW. A dean flow ultraviolet reactor was used with wavelength of 254 nm at the residence time of 14.0 seconds. The independent variables were three Reynold numbers (Re1 = 198.8, Re2 = 397.7 and Re3 =596.4) and two different diameters of transparent PFA tubes (3.2 mm and 1.6 mm). TCW was inoculated with cultures of Escherichia coli and Listeria monocytogenes separately up to 8 log10 CFU/mL and inactivation by cold pasteurization was evaluated with number of log reduction of each bacteria. Physico-chemical properties like total solid content (TSS) and pH were analyzed throughout the storage period of four weeks. The sensorial quality, flavor and color of the coconut water was also evaluated by a panel of 30 people to compare the organoleptic characteristics of UVC treated samples with untreated fresh coconut water. In case of Escherichia coli W1485, UVC treatment gave the log reduction of 5.27 and 4.74 log10 CFU/mL in coconut water for 1.6 mm and 3.2 mm ID reactors, respectively. Whereas the reduction of Listeria monocytogenes were 4.18 and 2.96 log10 CFU/mL for 1.6 mm and 3.2 mm ID reactors, respectively. In case of both the bacteria, as the tube size increased, microbial reduction decreased; and as the Reynold number increased, microbial reduction also increased except where there was an interaction effect. The change of tube diameters gave significantly different inactivation for both test bacteria at all Reynolds number except at Re2 and Re3 in case of Escherichia coli. The different levels of Reynolds number were not significantly variant when compared with consecutive levels, but Re1 to Re3 were significantly different for both test bacteria. The physico-chemical and sensorial changes of cold pasteurized TCW weres not significantly different compared to the fresh TCW, providing the conformity of retention of natural and organoleptic characteristics of TCW.

京都大学 / 新制・課程博士 / 博士(理学) / 甲第22995号 / 理博第4672号 / 新制||理||1670(附属図書館) / 京都大学大学院理学研究科物理学・宇宙物理学専攻 / (主査)教授 鶴 剛, 准教授 窪 秀利, 教授 中家 剛 / 学位規則第4条第1項該当 / Doctor of Science / Kyoto University / DFAM

The quasar 3C 279 was the target of an extensive multiwavelength monitoring campaign from 2006 January through April. An optical-IR-radio monitoring campaign by the Whole Earth Blazar Telescope (WEBT) collaboration was organized around target-of-opportunity X-ray and soft γ-ray observations with Chandra and INTEGRAL in 2006 mid-January, with additional X-ray coverage by RXTE and Swift XRT. In this paper we focus on the results of the WEBT campaign. The source exhibited substantial variability of optical flux and spectral shape, with a characteristic timescale of a few days. The variability patterns throughout the optical BVRI bands were very closely correlated with each other, while there was no obvious correlation between the optical and radio variability. After the ToO trigger, the optical flux underwent a remarkably clean quasi-exponential decay by about 1 mag, with a decay timescale of T d ∼ 12.8 days. In intriguing contrast to other (in particular, BL Lac type) blazars, we find a lag of shorter wavelength behind longer wavelength variability throughout the RVB wavelength ranges, with a time delay increasing with increasing frequency. Spectral hardening during flares appears delayed with respect to a rising optical flux. This, in combination with the very steep IR-optical continuum spectral index of α0 ∼ 1.5-2.0, may indicate a highly oblique magnetic field configuration near the base of the jet, leading to inefficient particle acceleration and a very steep electron injection spectrum. An alternative explanation through a slow (timescale of several days) acceleration mechanism would require an unusually low magnetic field of B ≲ 0.2 G, about an order of magnitude lower than inferred from previous analyses of simultaneous SEDs of 3C 279 and other flat-spectrum radio quasars with similar properties.