33 research outputs found

    Vacuum Expectation Value of the Higgs Field and Dyon Charge Quantisation from Spacetime Dependent Lagrangians

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    The spacetime dependent lagrangian formalism of references [1-2] is used to obtain is used to obtain a classical solution of Yang-Mills theory. This is then used to obtain an estimate of the vacuum expectation value of the Higgs field,{\it viz.} Ο•a=A/e\phi_{a}=A/e, where AA is a constant and ee is the Yang-Mills coupling (related to the usual electric charge).The solution can also accommodate non-commuting coordinates on the boundary of the theory which may be used to construct DD-brane actions. The formalism is also used to obtain the Deser-Gomberoff-Henneaux-Teitelboim results [10] for dyon charge quantisation in abelian pp-form theories in dimensions D=2(p+1)D=2(p+1) for both even and odd pp. PACS: 11.15.-q,11.27.+d,11.10.EfComment: Latex, 15 pages, a comprehensive paper incorporating material of hep-th/0210051, hence title and abstracts modified, typos correcte

    The Hawking temperature in the context of dark energy

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    An emergent gravity metric incorporating kβˆ’k-essence scalar fields Ο•\phi having a Born-Infeld type lagrangian is mapped into a metric whose structure is similar to that of a blackhole of large mass MM that has swallowed a global monopole. However, here the field is not that of a monopole but rather that of a kβˆ’k-essence scalar field. If Ο•emergent\phi_{emergent} be solutions of the emergent gravity equations of motion under cosmological boundary conditions at ∞\infty, then for rβ†’βˆžr\rightarrow\infty the rescaled field Ο•emergent2GMβˆ’1\frac {\phi_{emergent}}{2GM-1} has exact correspondence with Ο•\phi with Ο•(r,t)=Ο•1(r)+Ο•2(t)\phi(r,t)=\phi_{1}(r)+\phi_{2}(t). The Hawking temperature of this metric is Temergent=ℏc38Ο€GMkB(1βˆ’K)2≑ℏ8Ο€GMkB(1βˆ’K)2T_{\mathrm emergent}= \frac{\hbar c^{3}}{8\pi GM k_{\mathrm B}}(1-K)^{2}\equiv \frac{\hbar}{8\pi GM k_{\mathrm B}}(1-K)^{2}, taking the speed of light c=1c=1. Here K=Ο•Λ™22K=\dot\phi_{2}^{2} is the kinetic energy of the kβˆ’k-essence field Ο•\phi and KK is always less than unity, kBk_{\mathrm B} is the Boltzmann constant. This is phenomenologically interesting in the context of Belgiorno {\it et al's} gravitational analogue experiment.Comment: 6 pages, latex, To appear in Euro Physics Letters. arXiv admin note: text overlap with arXiv:1009.4634 by other author

    Three Flavoured neutrino oscillations and the Leggett Garg Inequality

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    Three flavoured neutrino oscillations are investigated in the light of the Leggett-Garg inequality. The outline of an experimental proposal is suggested whereby the findings of this investigation may be verified. The results obtained are: (a) The maximum violation of the Leggett Garg Inequality (LGI) is 2.170362.17036 for neutrino path length L1=140.15L_{1}=140.15 Km and Ξ”L=1255.7\Delta L=1255.7 Km.(b) Presence of the mixing angle ΞΈ13\theta_{13} enhances the maximum violation of LGI by 4.6%4.6\%.(c) The currently known mass hierarchy parameter Ξ±=0.0305\alpha = 0.0305 increases the the maximum violation of LGI by 3.7%3.7\%. (d)Presence of CP violating phase parameter enhances the maximum violation of LGI by 0.24%0.24\%, thus providing an \textit{alternative indicator of CP violation} in 3-flavoured neutrino oscillations.Comment: 8 pages, 5 figures, late
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