1,524 research outputs found
A Lagrange-D'Alembert formulation of the equations of motion of a helicopter carrying an externally suspended load
The exact nonlinear equations of motion are derived for a helicopter with an extenal load suspended by fore and aft, rigid-link cables. Lagrange's form of D'Alembert's principle is used. Ten degrees of freedom are necessary to represent the motion of this system in an inertial reference frame: six for the helicopter relative to inertial space and four for the load relative to the helicopter
LARGE-SCALE WIND-TUNNEL TESTS OF A CIRCULAR PLAN-FORM AIRCRAFT WITH A PERIPHERAL JET FOR LIFT, THRUST, AND CONTROL
Wind tunnel tests of circular planform aircraft with peripheral jet for lift, thrust, and contro
Equation of state sensitivities when inferring neutron star and dense matter properties
Understanding the dense matter equation of state at extreme conditions is an important open problem. Astrophysical observations of neutron stars promise to solve this, with NICER poised to make precision measurements of mass and radius for several stars using the waveform modelling technique. What has been less clear, however, is how these mass-radius measurements might translate into equation of state constraints and what are the associated equation of state sensitivities. We use Bayesian inference to explore and contrast the constraints that would result from different choices for the equation of state parametrization; comparing the well-established piecewise polytropic parametrization to one based on physically motivated assumptions for the speed of sound in dense matter. We also compare the constraints resulting from Bayesian inference to those from simple compatibility cuts. We find that the choice of equation of state parametrization and particularly its prior assumptions can have a significant effect on the inferred global mass-radius relation and the equation of state constraints. Our results point to important sensitivities when inferring neutron star and dense matter properties. This applies also to inferences from gravitational wave observations
The formation of the first galaxies and the transition to low-mass star formation
The formation of the first galaxies at redshifts z ~ 10-15 signaled the
transition from the simple initial state of the universe to one of ever
increasing complexity. We here review recent progress in understanding their
assembly process with numerical simulations, starting with cosmological initial
conditions and modelling the detailed physics of star formation. In this
context we emphasize the importance and influence of selecting appropriate
initial conditions for the star formation process. We revisit the notion of a
critical metallicity resulting in the transition from primordial to present-day
initial mass functions and highlight its dependence on additional cooling
mechanisms and the exact initial conditions. We also review recent work on the
ability of dust cooling to provide the transition to present-day low-mass star
formation. In particular, we highlight the extreme conditions under which this
transition mechanism occurs, with violent fragmentation in dense gas resulting
in tightly packed clusters.Comment: 16 pages, 7 figures, appeared in the conference proceedings for IAU
Symposium 255: Low-Metallicity Star Formation: From the First Stars to Dwarf
Galaxies, a high resolution version (highly recommended) can be found at
http://www.ita.uni-heidelberg.de/~tgreif/files/greif08.pd
Viable tax constitutions
Taxation is only sustainable if the general public complies with it. This observation is uncontroversial with tax practitioners but has been ignored by the public finance tradition, which has interpreted tax constitutions as binding contracts by which the power to tax is irretrievably conferred by individuals to government, which can then levy any tax it chooses. However, in the absence of an outside party enforcing contracts between members of a group, no arrangement within groups can be considered to be a binding contract, and therefore the power of tax must be sanctioned by individuals on an ongoing basis. In this paper we offer, for the first time, a theoretical analysis of this fundamental compliance problem associated with taxation, obtaining predictions that in some cases point to a re-interptretation of the theoretical constructions of the public finance tradition while in others call them into question
Glutamate Decarboxylases in Nonneural Cells of Rat Testis and Oviduct: Differential Expression of GAD 65 and GAD 67
Γ-Aminobutyric acid (GABA) and its synthetic enzyme, glutamate decarboxylase (GAD), are not limited to the nervous system but are also found in nonneural tissues. The mammalian brain contains at least two forms of GAD (GAD 67 and GAD 65 ), which differ from each other in size, sequence, immunoreactivity, and their interaction with the cofactor pyridoxal 5′-phosphate (PLP). We used cDNAs and antibodies specific to GAD 65 and GAD 67 to study the molecular identity of GADs in peripheral tissues. We detected GAD and GAD mRNAs in rat oviduct and testis. In oviduct, the size of GAD, its response to PLP, its immunoreactivity, and its hybridization to specific RNA and DNA probes all indicate the specific expression of the GAD 65 gene. In contrast, rat testis expresses the GAD 67 gene. The GAD in these two reproductive tissues is not in neurons but in nonneural cells. The localization of brain GAD and GAD mRNAs in the mucosal epithelial cells of the oviduct and in spermatocytes and spermatids of the testis shows that GAD is not limited to neurons and that GABA may have functions other than neurotransmission.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/66211/1/j.1471-4159.1992.tb09763.x.pd
Influence of Population III stars on cosmic chemical evolution
New observations from the Hubble ultra deep field suggest that the star
formation rate at z>7 drops off faster than previously thought. Using a newly
determined star formation rate for the normal mode of Population II/I stars
(PopII/I), including this new constraint, we compute the Thomson scattering
optical depth and find a result that is marginally consistent with WMAP5
results. We also reconsider the role of Population III stars (PopIII) in light
of cosmological and stellar evolution constraints. While this input may be
needed for reionization, we show that it is essential in order to account for
cosmic chemical evolution in the early Universe. We investigate the
consequences of PopIII stars on the local metallicity distribution function of
the Galactic halo (from the recent Hamburg/ESO survey of metal-poor stars) and
on the evolution of abundances with metallicity (based on the ESO large program
on very metal-poor stars), with special emphasis on carbon-enhanced metal-poor
stars. Our most important results show that the nucleosynthetic yields of
PopIII stars lead to abundance patterns in agreement with those observed in
extremely metal-poor stars. In this chemical approach to cosmic evolution,
PopIII stars prove to be a compulsory ingredient, and extremely metal-poor
stars are inevitably born at high redshift. (Abridged)Comment: 11 pages, 7 figures, MNRAS in pres
A remembrance of things (best) forgotten: The 'allegorical past' and the feminist imagination
This is the author's PDF version of an article published in Feminist theology© 2012. The definitive version is available at http://fth.sagepub.com/This article discusses the US TV series Mad Men, which is set in an advertising agency in 1960s New York, in relation to two key elements which seem significant for a consideration of the current state of feminism in church and academy, both of which centre around what it means to remember or (not) to forget
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