13,643 research outputs found

    The Stability of Branonium

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    We analyse the orbital motion of a light anti D6-brane in the presence of a stack of heavy, distant D6-branes in ten dimensions, taking account of possible time-variations in the background moduli fields. The Coulomb-like central potential arising through brane-antibrane interactions is then modified to include time-dependent prefactors, which generally preclude the existence of stable elliptical orbits.Comment: 13 pages, Latex, 3 eps figure

    The Hamilton-Waterloo Problem with even cycle lengths

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    The Hamilton-Waterloo Problem HWP(v;m,n;α,β)(v;m,n;\alpha,\beta) asks for a 2-factorization of the complete graph KvK_v or KvIK_v-I, the complete graph with the edges of a 1-factor removed, into α\alpha CmC_m-factors and β\beta CnC_n-factors, where 3m<n3 \leq m < n. In the case that mm and nn are both even, the problem has been solved except possibly when 1{α,β}1 \in \{\alpha,\beta\} or when α\alpha and β\beta are both odd, in which case necessarily v2(mod4)v \equiv 2 \pmod{4}. In this paper, we develop a new construction that creates factorizations with larger cycles from existing factorizations under certain conditions. This construction enables us to show that there is a solution to HWP(v;2m,2n;α,β)(v;2m,2n;\alpha,\beta) for odd α\alpha and β\beta whenever the obvious necessary conditions hold, except possibly if β=1\beta=1; β=3\beta=3 and gcd(m,n)=1\gcd(m,n)=1; α=1\alpha=1; or v=2mn/gcd(m,n)v=2mn/\gcd(m,n). This result almost completely settles the existence problem for even cycles, other than the possible exceptions noted above

    Brane Gases on K3 and Calabi-Yau Manifolds

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    We initiate the study of Brane Gas Cosmology (BGC) on manifolds with non-trivial holonomy. Such compactifications are required within the context of superstring theory in order to make connections with realistic particle physics. We study the dynamics of brane gases constructed from various string theories on background spaces having a K3 submanifold. The K3 compactifications provide a stepping stone for generalising the model to the case of a full Calabi-Yau three-fold. Duality symmetries are discussed within a cosmological context. Using a duality, we arrive at an N=2 theory in four-dimensions compactified on a Calabi-Yau manifold with SU(3) holonomy. We argue that the Brane Gas model compactified on such spaces maintains the successes of the trivial toroidal compactification while greatly enhancing its connection to particle physics. The initial state of the universe is taken to be a small, hot and dense gas of p-branes near thermal equilibrium. The universe has no initial singularity and the dynamics of string winding modes allow three spatial dimensions to grow large, providing a possible solution to the dimensionality problem of string theory.Comment: 26 pages; Significant revisions: review material truncated; presentation improve

    Study of space cabin atmospheres Status report, Jul. 1 - Dec. 31, 1967

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    Calibration of hot-wire detector for particle concentration and size distribution in closed spacecraft cabin atmosphere

    Study of Space Cabin Atmospheres Status Report, 1 Jan. - 30 Jun. 1966

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    Performance characteristics of aerosol generator, and distribution sampling errors of electrostatic precipitator sampling device for space cabin atmospher

    The high partial wave phenomenon of spin changing atomic transitions

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    The collisional transition between two highly excited atomic states with different spin is investigated theoretically. Taking helium-like n1S − n3P as an example, it is found that the transition is driven in the highly ion-ized Fe ion purely by exchange, and the cross section becomes increasingly dominated by partial waves of high orbital angular momentum as the scattering energy increases. Whereas for the near-neutral Li ion the transition is dominated by channel coupling in low partial waves. Analytical bench-marks and numerical methods are developed for the accurate calculation of the exchange integral at high angular momentum. It is shown how the partial wave and energy dependence of the collision strength for high n spin changing transitions in the highly ionized ion is related to the overlap of the extended atomic orbitals.</p
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