Tracing the atomic nitrogen abundance in star-forming regions with ammonia deuteration

Partitioning of elemental nitrogen in star-forming regions is not well constrained. Most nitrogen is expected to be partitioned among atomic nitrogen, molecular nitrogen (N2), and icy N-bearing molecules, such as ammonia (NH3) and N2. Atomic nitrogen is not directly observable in the cold gas. In this paper, we propose an indirect way to constrain the amount of atomic nitrogen in the cold gas of star-forming clouds, via deuteration in ammonia ice, the [ND2H/NH2D]/[NH2D/NH3] ratio. Using gas-ice astrochemical simulations, we show that if atomic nitrogen remains as the primary reservoir of nitrogen during cold ice formation stages, the [ND2H/NH2D]/[NH2D/NH3] ratio is close to the statistical value of 1/3 and lower than unity, whereas if atomic nitrogen is largely converted into N-bearing molecules, the ratio should be larger than unity. Observability of ammonia isotopologues in the inner hot regions around low-mass protostars, where ammonia ice has sublimated, is also discussed. We conclude that the [ND2H/NH2D]/[NH2D/NH3] ratio can be quantified using a combination of VLA and ALMA observations with reasonable integration times, at least toward IRAS 16293-2422 where high molecular column densities are expected.Comment: Accepted for publication in MNRAS, 12 pages, 9 figures, 1 Tabl

The Effects on Sick Leave of Changes in the Sickness Insurance System

In order to get a more complete picture of how labor supply is affected by economic incentives, the effects on absenteeism and not just on contracted hours should be taken into account. In particular, absenteeism due to sick leave can be considerable. In this paper we examine whether the level of sick leave compensation affects sick leave behavior. Using time-series data for Sweden spanning a long period (1955–99) with numerous changes of the compensation level, we generally find strong effects of the expected sign. Reforms implying more generous compensation for sick leave tend to be associated with permanent increases in total sick leave per person employed and vice versa. These findings are reinforced in a panel study covering the 1983–91 period.Absenteeism; Labor supply; Sick leave; Sickness insurance; Social security

Highly loaded HPT blading in KTH test turbine - An attempt to reduce the number of blades in the first stage in a high pressure turbine

The main goal with this thesis was to investigate the possibility to reduce the number of blades in a high pressure gas turbine row. The reason for this study was the interest to reduce the amount of cooling air needed within the blade row by reducing the wetted area, hopefully without losing efficiency. Another reason for reducing the number of blades was to reduce the costs. A new design of an uncooled scaled model blade for a first stage blade row in a modern industrial gas turbine was developed. The design process mixed a combination of new ideas and more proven design principles of Siemens Industrial Turbomachinery AB. The new blade row was designed so it would fit in the existing test turbine at the Royal Institute of Technology in Stockholm. This new blade row containing 50 blades was then compared to the existing BC7M blade row which has 60 blades. By the use of Siemens in-house codes beta2, MAC1, Multall and Cato such parameters as efficiency, Zweifel coefficient, degree of reaction and losses were studied. The final design of the new blade resulted in a reduction of the blades combined wetted area by 9320 mm2 or 9.7 %, this without losing more than 0.12 percentage efficiency from 92.02 % to 91.90 % according to the Multall results. According to the beta2 results the efficiency increased with 0.16 percentage from 92.03 % to 92.19 %. The profile hub-section area has though decreased by 1276 mm2 or 20.4 % which means that this extra uncovered platform wetted area on the rotor may need cooling. Even though these numbers appear to be good, some problem has to be solved before being able to manufacture this new blade row, e.g. the stagnation point at the leading edge, especially at the tip-section occurs on the pressure side. This will not be a problem for this uncooled model. However in case of a cooled full scale design, the shower head cooling at the leading edge will end up on the suction side, which may result in an overheated pressure side. Of course a structural analysis should be done as well

Nanowire Transistors and RF Circuits for Low-Power Applications

The background of this thesis is related to the steadily increasing demand of higher bandwidth and lower power consumption for transmitting data. The work aims at demonstrating how new types of structures, at the nanoscale, combined with what is referred to as exotic materials, can help benefit in electronics by lowering the consumed power, possibly by an order of magnitude, compared to the industry standard, silicon (Si), used today. Nanowires are semiconductor rods, with two dimensions at the nanoscale, which can be either grown with a bottom-up technique, or etched out with a top-down approach. The research interest concerning nanowires has gradually increasing for over two decades. Today, few have doubts that nanowires represent an attractive alternative, as scaling of planar structures has reached fundamental limits. With the enhanced electrostatics of a surrounding gate, nanowires offer the possibility of continued miniaturization, giving semiconductors a prolonged window of performance improvements. As a material choice, compound semiconductors with elements from group III and V (III-Vs), such as indium arsenide (InAs), have the possibility to dramatically decrease power consumption. The reason is the inherent electron transport properties of III-Vs, where an electron can travel, in the order of, 10 times faster than in Si. In the projected future, inclusion of III-Vs, as an extension to the Si-CMOS platform, seems almost inevitable, with many of the largest electronics manufacturing companies showing great interest. To investigate the technology potential, we have fabricated InAs nanowire metal-oxide-semiconductor field effect transistors (NW-FETs). The performance has been evaluated measuring both RF and DC characteristics. The best devices show a transconductance of 1.36 mS/µm (a device with a single nanowire, normalized to the nanowire circumference) and a maximum unilateral power gain at 57 GHz (for a device with several parallel nanowires), both values at a drive voltage of 0.5 V. The performance metrics are found to be limited by the capacitive load of the contact pads as well as the resistance in the non-gated segments of the nanowires. Using computer models, we have also been able to extract intrinsic transport properties, quantifying the velocity of charge carrier injection, which is the limiting property of semi-ballistic and ballistic devices. The value for our 45-nm-in-diameter nanowires, with 200 nm channel length, is determined to 1.7∙107 cm/s, comparable to other state-of-the-art devices at the same channel length. To demonstrate a higher level of functionality, we have connected several NW-FETs in a circuit. The fabricated circuit is a single balanced differential direct conversion mixer and is composed of three stages; transconductance, mixing, and transimpedance. The basic idea of the mixer circuit is that an information signal can either be extracted from or inserted into a carrier wave at a higher frequency than the information wave itself. It is the relative size of the first and the third stage that accounts for the circuit conversion gain. Measured circuits show a voltage conversion gain of 6 dB and a 3-dB bandwidth of 2 GHz. A conversion mixer is a vital component when building a transceiver, like those found in a cellphone and any other type of radio signal transmitting device. For all types of signals, noise imposes a fundamental limitation on the minimal, distinguishable amplitude. As transistors are scaled down, fewer carriers are involved in charge transport, and the impact of frequency dependent low-frequency noise gets relatively larger. Aiming towards low power applications, it is thus of importance to minimize the amount of transistor generated noise. Included in the thesis are studies of the level and origin of low-frequency 1/f-noise generated in NW-FETs. The measured noise spectral density is comparable to other non-planar devices, including those fabricated in Si. The data suggest that the level of generated noise can be substantially lowered by improving the high-k dielectric film quality and the channel interface. One significant discovery is that the part of the noise originating from the bulk nanowire, identified as mobility fluctuations, is comparably much lower than the measured noise level related to the nanowire surface. This result is promising as mobility fluctuations set the lower limit of what is achievable within a material system

Warm water deuterium fractionation in IRAS 16293-2422 - The high-resolution ALMA and SMA view

Measuring the water deuterium fractionation in the inner warm regions of low-mass protostars has so far been hampered by poor angular resolution obtainable with single-dish ground- and space-based telescopes. Observations of water isotopologues using (sub)millimeter wavelength interferometers have the potential to shed light on this matter. Observations toward IRAS 16293-2422 of the 5(3,2)-4(4,1) transition of H2-18O at 692.07914 GHz from Atacama Large Millimeter/submillimeter Array (ALMA) as well as the 3(1,3)-2(2,0) of H2-18O at 203.40752 GHz and the 3(1,2)-2(2,1) transition of HDO at 225.89672 GHz from the Submillimeter Array (SMA) are presented. The 692 GHz H2-18O line is seen toward both components of the binary protostar. Toward one of the components, "source B", the line is seen in absorption toward the continuum, slightly red-shifted from the systemic velocity, whereas emission is seen off-source at the systemic velocity. Toward the other component, "source A", the two HDO and H2-18O lines are detected as well with the SMA. From the H2-18O transitions the excitation temperature is estimated at 124 +/- 12 K. The calculated HDO/H2O ratio is (9.2 +/- 2.6)*10^(-4) - significantly lower than previous estimates in the warm gas close to the source. It is also lower by a factor of ~5 than the ratio deduced in the outer envelope. Our observations reveal the physical and chemical structure of water vapor close to the protostars on solar-system scales. The red-shifted absorption detected toward source B is indicative of infall. The excitation temperature is consistent with the picture of water ice evaporation close to the protostar. The low HDO/H2O ratio deduced here suggests that the differences between the inner regions of the protostars and the Earth's oceans and comets are smaller than previously thought.Comment: Accepted for publication in Astronomy & Astrophysic

Context-aware adaptation in DySCAS

DySCAS is a dynamically self-configuring middleware for automotive control systems. The addition of autonomic, context-aware dynamic configuration to automotive control systems brings a potential for a wide range of benefits in terms of robustness, flexibility, upgrading etc. However, the automotive systems represent a particularly challenging domain for the deployment of autonomics concepts, having a combination of real-time performance constraints, severe resource limitations, safety-critical aspects and cost pressures. For these reasons current systems are statically configured. This paper describes the dynamic run-time configuration aspects of DySCAS and focuses on the extent to which context-aware adaptation has been achieved in DySCAS, and the ways in which the various design and implementation challenges are met

Support and opposition in an attempted higher education merger

The study explores an ultimately unsuccessful merger of three Norwegian public university colleges. It shows how social practices of support for and opposition to the merger were the effects of the intersection(s) between why the merger was necessary and how the proposed merger process was enacted. Support and opposition may change during the merger process, since participants move in and out of positions given how the process unfolds. We relate support and opposition to identity. A merger supports attractive identities if it is consonant with overarching normative ideals of higher education and experienced fairness during the merger process. The findings have implications for how we can better understand and explain why some merger initiatives lead to termination instead of a merger.publishedVersio