22,219 research outputs found

    Bulk matter fields on two-field thick branes

    Full text link
    In this paper we obtain a new solution of a brane made up of a scalar field coupled to a dilaton. There is a unique parameter bb in the solution, which decides the distribution of the energy density and will effect the localization of bulk matter fields. For free vector fields, we find that the zero mode can be localized on the brane. And for vector fields coupled with the dilaton via eτπFMNFMN\text{e}^{\tau\pi}F_{MN}F^{MN}, the condition for localizing the zero mode is τ≥−b/3\tau\geq-\sqrt{b/3} with 0−1/3b0-1/\sqrt{3b} with b>1b>1, which includes the case τ=0\tau=0. While the zero mode for free Kalb-Ramond fields can not be localized on the brane, if only we introduce a coupling between the Kalb-Ramond fields and the dilaton via eζπHMNLHMNL\text{e}^{\zeta \pi}H_{MNL}H^{MNL}. When the coupling constant satisfies ζ>1/3b\zeta>1/\sqrt{3b} with b≥1b\geq1 or ζ>2−b3b\zeta>\frac{2-b}{\sqrt{3b}} with 0<b<10<b<1, the zero mode for the KR fields can be localized on the brane. For spin half fermion fields, we consider the coupling ηΨˉeλπϕΨ\eta\bar{\Psi}\text{e}^{\lambda \pi}\phi\Psi between the fermions and the background scalars with positive Yukawa coupling η\eta. The effective potentials for both chiral fermions have three types of shapes decided by the relation between the dilaton-fermion coupling constant λ\lambda and the parameter bb. For λ≤−1/3b\lambda\leq-1/\sqrt{3b}, the zero mode of left-chiral fermion can be localized on the brane. While for λ>−1/3b\lambda>-1/\sqrt{3b} with b>1b>1 or −1/3b<λ<−b/3-1/\sqrt{3b}<\lambda<-\sqrt{b/3} with 0<b≤10<b\leq1, the zero mode for left-chiral fermion also can be localized.Comment: 22 pages, 8 figures, improved version, accepted by Physical Review

    Gravity Localization and Effective Newtonian Potential for Bent Thick Branes

    Full text link
    In this letter, we first investigate the gravity localization and mass spectrum of gravity KK modes on de Sitter and Anti-de Sitter thick branes. Then, the effective Newtonian gravitational potentials for these bent branes are discussed by the two typical examples. The corrections of the Newtonian potential turns out to be ΔU(r)∼1/r2\Delta U(r)\sim 1/r^{2} at small rr for both cases. These corrections are very different from that of the Randall-Sundrum brane model ΔU(r)∼1/r3\Delta U(r)\sim 1/r^{3}.Comment: 6 pages, 2 figure
    • …
    corecore