5,793 research outputs found

    Space-suit carbon dioxide absorption system: A concept

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    Partial pressure of carbon dioxide within a space suit is maintained at safe levels by regenerating carbon dioxide with potassium hydroxide solution on board spacecraft or by portable units

    Instrument calibrates low gas-rate flowmeters

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    Electronically measuring the transit time of a soap bubble carried by the gas stream between two fixed points in a burette calibrates flowmeters used for measuring low gas-flow rates

    Ground state of high-density matter

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    It is shown that if an upper bound to the false vacuum energy of the electroweak Higgs potential is satisfied, the true ground state of high-density matter is not nuclear matter, or even strange-quark matter, but rather a non-topological soliton where the electroweak symmetry is exact and the fermions are massless. This possibility is examined in the standard SU(3) sub C tensor product SU(2) sub L tensor product U(1) sub Y model. The bound to the false vacuum energy is satisfied only for a narrow range of the Higgs boson masses in the minimal electroweak model (within about 10 eV of its minimum allowed value of 6.6 GeV) and a somewhat wider range for electroweak models with a non-minimal Higgs sector

    Constraints on string networks with junctions

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    We consider the constraints on string networks with junctions in which the strings may all be different, as may be found for example in a network of (p,q)(p,q) cosmic superstrings. We concentrate on three aspects of junction dynamics. First we consider the propagation of small amplitude waves across a static three-string junction. Then, generalizing our earlier work, we determine the kinematic constraints on two colliding strings with different tensions. As before, the important conclusion is that strings do not always reconnect with a third string; they can pass straight through one another (or in the case of non-abelian strings become stuck in an X configuration), the constraint depending on the angle at which the strings meet, on their relative velocity, and on the ratios of the string tensions. For example, if the two colliding strings have equal tensions, then for ultra-relativistic initial velocities they pass through one another. However, if their tensions are sufficiently different they can reconnect. Finally, we consider the global properties of junctions and strings in a network. Assuming that, in a network, the incoming waves at a junction are independently randomly distributed, we determine the r.m.s. velocities of strings and calculate the average speed at which a junction moves along each of the three strings from which it is formed. Our findings suggest that junction dynamics may be such as to preferentially remove the heavy strings from the network leaving a network of predominantly light strings. Furthermore the r.m.s. velocity of strings in a network with junctions is smaller than 1/\sqrt{2}, the result for conventional Nambu-Goto strings without junctions in Minkowski spacetime.Comment: 12 pages, 6 figures. Version to appear in PRD. (2 new references and slightly extended discussion in section VII

    Reheating and gravitino production in braneworld inflation

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    We consider the constraints that can be imposed on a wide class of Inflation models in modified gravity scenarios in which the Friedmann equation is modified by the inclusion of ρ2\rho^2 terms, where ρ\rho is the total energy density. In particular we obtain the reheating temperature and gravitino abundance associated with the end of inflation. Whereas models of chaotic inflation and natural inflation can easily avoid the conventional gravitino overproduction problem, we show that supersymmetric hybrid inflation models (driven by both F and D-terms) do not work in the ρ2\rho^2 dominated era. We also study inflation driven by exponetial potentials in this modified background, and show that the gravitino production is suppressed enough to avoid there being a problem, although other conditions severely constrain these models.Comment: 24page

    Heir Property in the African American Community: From Promised Lands to Problem Lands

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    Abstract African American landowners have been reluctant to take advantage of intergenerational succession laws which provide for an orderly transfer of property from one generation to the next. This reluctance has led to a prevalence of heir property. Heir property is created when a person dies intestate. Heir property has created an impediment to wealth accumulation and has contributed to African American land loss in America. Partition actions are a byproduct of heir property which has operated to accelerate the loss of real property in the African American community. The Uniform Partition of Heir Property Act provides for procedural safeguards that would allow for cotenants of heir property to buy out other heirs and provide more discernable notices of partition actions. These factors will likely militate against the precipitous loss of African American lands due to partition lawsuits initiated because of heir property. Keywords: Heir Property, Partition, Land Loss, Interstate Successio

    The Magnificent Purpose

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    Management by objectives: a model for the local Wesleyan Church

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    https://place.asburyseminary.edu/ecommonsatsdissertations/1020/thumbnail.jp

    Charles Alexander Eastman (Ohiyesa)

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    Because Charles Eastman’s best known book is his earliest, Indian Boyhood (1902), and because that autobiography and its sequel, From the Deep Woods to Civilization (1916), have been most often used as sources for studies of the cultural transition of the Sioux, the literary value of those and of Eastman’s later books has gone largely unexamined. Eastman subtitled the 1916 volume The Autobiography of an Indian, but one cannot therefore assume that the conventions of European-American autobiography control Eastman’s work
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