4,776 research outputs found

    Latitudinal Shear Instabilities during Type I X-ray Bursts

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    Coherent oscillations have been observed during Type I X-ray bursts from 14 accreting neutron stars in low mass X-ray binaries, providing important information about their spin frequencies. However, the origin of the brightness asymmetry on the neutron star surface producing these oscillations is still not understood. We study the stability of a zonal shearing flow on the neutron star surface using a shallow water model. We show that differential rotation of >2% between pole and equator, with the equator spinning faster than the poles, is unstable to hydrodynamic shear instabilities. The unstable eigenmodes have properties well-matched to burst oscillations: low azimuthal wavenumber m, wave speeds 1 or 2% below the equatorial spin rate, and e-folding times close to a second. Instability is related to low frequency buoyantly driven r-modes that have a mode frequency within the range of rotation frequencies in the differentially rotating shell. We discuss the implications for burst oscillations. Growth of shear instabilities may explain the brightness asymmetry in the tail of X-ray bursts, although some fine tuning of the level of differential rotation and a spin frequency near 300 Hz are required in order for the fastest growing mode to have m=1. If shear instabilities are to operate during a burst, temperature contrasts of 30% across the star must be created during ignition and spreading of the flash.Comment: To appear in ApJ (12 pages, 11 figures

    Experimentally estimated dead space for GaAs and InP based planar Gunn diodes

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    The authors would like to thank the staff of the James Watt Nanofabrication Centre at the University of Glasgow for help in fabricating the devices which is reported in this paper. ā€˜Part of this work was supported by ESPRC through EP/H011862/ 1, and EP/H012966/1.Peer reviewedPublisher PD

    The Nondual Mind: Vedānta, Kashmiri PratyabhijƱā Shaivism, and Spinoza

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    This book compares Hindu nondual philosophy to that of Baruch Spinoza, demonstrating the similarity of Spinoza's ideas to Kashmiri PratyabhijƱā Shaivism. The book is well researched, but it is written in an informal style suitable for both scholars and the educated general public. There is already some scholarly literature comparing Spinoza's philosophy to Śaį¹…kara's Vedānta, but none of it has focused, as this book does, on philosophy of mind, and none of it has included Kashmiri Shaivism in the comparison. Among other things, the important distinction between Śaį¹…kara's Vedānta and Kashmiri Shaivism is brought to the fore by looking at those two philosophies through the lens of Spinoza. The primary focus of the book is the question of consciousness, but one cannot explain consciousness without also saying something about ontology, epistemology, determinism, ethics, and death. The book dispels the illusion of the subject-object divide, which is the primary source of confusion for many philosophy-of-mind scholars. And when the illusion of the subject-object divide dissolves, the mind-body problem dissolves with it, and philosophical puzzles like Mary and her black-and-white room are easily solved. The key point is that all consciousness is consciousness of one's own self. One cannot be conscious of a thing ā€” anything ā€” withoutĀ beingĀ that thing. The reason there appears to be an outside world, when in truth one is only consciousness of one's own self, is the same reason that the reflection of a city on the flat surface of a small mirror appears to be a distant city. It is a trick of perception that makes one's consciousness of self appear to be the knowing of an external world. But even more important, consciousness of self is not different from being self, for consciousness and being are the same thing. This book will appeal to philosophy of mind scholars, and it will thrill students of South Asian nondualism. But it is worth reading just for the brief anecdote about Einstein in Princeton and what that anecdote tells us about human agency

    The Value of Pi in the Bible (And What It Tells Us about Biblical Hermeneutics)

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    This two-page essay provides intriguing evidence that the Bible was encoded by its original redactors

    What makes the Crab pulsar shine?

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    Our high time resolution observations of individual pulses from the Crab pulsar show that the main pulse and interpulse differ in temporal behavior, spectral behavior, polarization and dispersion. The main pulse properties are consistent with one current model of pulsar radio emission, namely, soliton collapse in strong plasma turbulence. The high-frequency interpulse is quite another story. Its dynamic spectrum cannot easily be explained by any current emission model; its excess dispersion must come from propagation through the star's magnetosphere. We suspect the high-frequency interpulse does not follow the ``standard model'', but rather comes from some unexpected region within the star's magnetosphere. Similar observations of other pulsars will reveal whether the radio emission mechanisms operating in the Crab pulsar are unique to that star, or can be identified in the general population.Comment: 5 pages, 2 figures, to appear in proceedings of meeting "Forty Years of Pulsars: Millisecond Pulsars, Magnetars and More", Montreal, August 200

    A bibliography of published information relevant to fire toxicity

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    A bibliography containing 883 references in the field of fire toxicity is presented to assist in literature searches to help reduce human fire hazards

    Impact ionisation electroluminescence in planar GaAs-based heterostructure Gunn diodes:Spatial distribution and impact of doping nonuniformities

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    When biased in the negative differential resistance regime, electroluminescence (EL) is emitted from planar GaAs heterostructure Gunn diodes. This EL is due to the recombination of electrons in the device channel with holes that are generated by impact ionisation when the Gunn domains reach the anode edge. The EL forms non-uniform patterns whose intensity shows short-range intensity variations in the direction parallel to the contacts and decreases along the device channel towards the cathode. This paper employs Monte Carlo models, in conjunction with the experimental data, to analyse these non-uniform EL patterns and to study the carrier dynamics responsible for them. It is found that the short-range lateral (i.e., parallel to the device contacts) EL patterns are probably due to non-uniformities in the doping of the anode contact, illustrating the usefulness of EL analysis on the detection of such inhomogeneities. The overall decreasing EL intensity towards the anode is also discussed in terms of the interaction of holes with the time-dependent electric field due to the transit of the Gunn domains. Due to their lower relative mobility and the low electric field outside of the Gunn domain, freshly generated holes remain close to the anode until the arrival of a new domain accelerates them towards the cathode. When the average over the transit of several Gunn domains is considered, this results in a higher hole density, and hence a higher EL intensity, next to the anode
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