7,398 research outputs found

    QED in strong, finite-flux magnetic fields

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    Lower bounds are placed on the fermionic determinants of Euclidean quantum electrodynamics in two and four dimensions in the presence of a smooth, finite-flux, static, unidirectional magnetic field B(r)=(0,0,B(r))B(r) =(0,0,B(r)), where B(r)0B(r) \geq 0 or B(r)0B(r) \leq 0, and rr is a point in the xy-plane.Comment: 10 pages, postscript (in uuencoded compressed tar file

    Failure of the Standard Coupled-Channels Method in Describing the Inelastic Reaction Data: On the Use of a New Shape for the Coupling Potential

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    We present the failure of the standard coupled-channels method in explaining the inelastic scattering together with other observables such as elastic scattering, excitation function and fusion data. We use both microscopic double-folding and phenomenological deep potentials with shallow imaginary components. We argue that the solution of the problems for the inelastic scattering data is not related to the central nuclear potential, but to the coupling potential between excited states. We present that these problems can be addressed in a systematic way by using a different shape for the coupling potential instead of the usual one based on Taylor expansion.Comment: 10 pages, 4 figures, 1 table, Latex:RevTex4 published in J. Phys. G: Nucl. Part. Phy

    Constraints on Galaxy Bias, Matter Density, and Primordial Non--Gausianity from the PSCz Galaxy Redshift Survey

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    We compute the bispectrum for the \IRAS PSCz catalog and find that the galaxy distribution displays the characteristic signature of gravity. Assuming Gaussian initial conditions, we obtain galaxy biasing parameters 1/b1=1.200.19+0.181/b_1=1.20^{+0.18}_{-0.19} and b2/b12=0.42±0.19b_2/b_1^2=-0.42\pm0.19, with no sign of scale-dependent bias for k0.3k\leq 0.3 h/Mpc. These results impose stringent constraints on non-Gaussian initial conditions. For dimensional scaling models with χN2\chi^2_N statistics, we find N>49, which implies a constraint on primordial skewness B3<0.35B_3<0.35.Comment: 4 pages, 3 embedded figures, uses revtex style file, minor changes to reflect published versio

    Mass zeros in the one-loop effective actions of QED in 1+1 and 3+1 dimensions

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    It is known that the one-loop effective action of QED2{QED}_2 is a quadratic in the field strength when the fermion mass is zero: all potential higher order contributions beyond second order vanish. For nonzero fermion mass it is shown that this behavior persists for a general class of fields for at least one value of the fermion mass when the external field's flux Φ\Phi satisfies 0<eΦ<2π0<|e\Phi|<2\pi. For QED4{QED}_4 the mass-shell renormalized one-loop effective action vanishes for at least one value of the fermion mass for a class of smooth, square integrable background gauge fields provided a plausible zero-mass limit exists.Comment: Section IV has been amende

    Fermionic Determinant of the Massive Schwinger Model

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    A representation for the fermionic determinant of the massive Schwinger model, or QED2QED_2, is obtained that makes a clean separation between the Schwinger model and its massive counterpart. From this it is shown that the index theorem for QED2QED_2 follows from gauge invariance, that the Schwinger model's contribution to the determinant is canceled in the weak field limit, and that the determinant vanishes when the field strength is sufficiently strong to form a zero-energy bound state

    Protecting the Primordial Baryon Asymmetry From Erasure by Sphalerons

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    If the baryon asymmetry of the universe was created at the GUT scale, sphalerons together with exotic sources of (BL)(B-L)-violation could have erased it, unless the latter satisfy stringent bounds. We elaborate on how the small Yukawa coupling of the electron drastically weakens previous estimates of these bounds.Comment: 41 pp., 4 latex figures included and 3 uuencoded or postscript figures available by request, UMN-TH-1213-9

    Anomalous quantum confined Stark effects in stacked InAs/GaAs self-assembled quantum dots

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    Vertically stacked and coupled InAs/GaAs self-assembled quantum dots (SADs) are predicted to exhibit a strong non-parabolic dependence of the interband transition energy on the electric field, which is not encountered in single SAD structures nor in other types of quantum structures. Our study based on an eight-band strain-dependent kp{\bf k}\cdot{\bf p} Hamiltonian indicates that this anomalous quantum confined Stark effect is caused by the three-dimensional strain field distribution which influences drastically the hole states in the stacked SAD structures.Comment: 4 pages, 4 figure

    Leptogenesis with Dirac Neutrinos

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    We describe a "neutrinogenesis" mechanism whereby, in the presence of right-handed neutrinos with sufficiently small pure Dirac masses, (B+L)-violating sphaleron processes create the baryon asymmetry of the Universe, even when B=L=0 initially. It is shown that the resulting neutrino mass constraints are easily fulfilled by the neutrino masses suggested by current experiments. We present a simple toy model which uses this mechanism to produce the observed baryon asymmetry of the Universe. (PostScript Errors corrected in latest Version).Comment: 4 pages, Latex (using amsmath,feynmp,graphicx), 4 figure

    The Ursinus Weekly, October 13, 1905

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    School of Theology • Football • Oyster supper • Society notes • College notes • Alumni • Ursinus Union • College world • Camp reunion • Literary Supplement: A plea for the children; Cut from life; Ludwig van Beethoven; Youth\u27s passion; A distinctive American literature; Experience of a View Agent; Carpe diem; Integrity in political life • Exchangeshttps://digitalcommons.ursinus.edu/weekly/2952/thumbnail.jp

    Gravitino constraints on models of neutrino masses and leptogenesis

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    In the supersymmetric extensions of the standard model, neutrino masses and leptogenesis requires existence of new particles. We point out that if these particles with lepton number violating interactions have standard model gauge interactions, then they may not be created after reheating because of the gravitino problem. This will rule out all existing models of neutrino masses and leptogenesis, except the one with right-handed singlet neutrinos.Comment: 12 pages latex file with one postscript figur
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