6,774 research outputs found

    Constraints on the Brans-Dicke gravity theory with the Planck data

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    Based on the new cosmic CMB temperature data from the Planck satellite, the 9 year polarization data from the WMAP, the BAO distance ratio data from the SDSS and 6dF surveys, we place a new constraint on the Brans-Dicke theory. We adopt a parametrization \zeta=\ln(1+1/\omega}), where the general relativity (GR) limit corresponds to ΞΆ=0\zeta = 0. We find no evidence of deviation from general relativity. At 95% probability, βˆ’0.00246<ΞΆ<0.00567-0.00246 < \zeta < 0.00567, correspondingly, the region βˆ’407.0<Ο‰<175.87-407.0 < \omega <175.87 is excluded. If we restrict ourselves to the ΞΆ>0\zeta>0 (i.e. Ο‰>0\omega >0) case, then the 95% probability interval is ΞΆ181.65\zeta 181.65. We can also translate this result to a constraint on the variation of gravitational constant, and find the variation rate today as GΛ™=βˆ’1.42βˆ’2.27+2.48Γ—10βˆ’13\dot{G}=-1.42^{+2.48}_{-2.27} \times 10^{-13} yrβˆ’1^{-1} (1Οƒ1\sigma error bar), the integrated change since the epoch of recombination is Ξ΄G/G=0.0104βˆ’0.0067+0.0186\delta G/G = 0.0104^{+0.0186}_{-0.0067} (1Οƒ1\sigma error bar). These limits on the variation of gravitational constant are comparable with the precision of solar system experiments.Comment: 7 pages, 5 figures, 2 table

    Thermodynamics in the universe described by the emergence of the space and the energy balance relation

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    It has previously been shown that it is more general to describe the evolution of the universe based on the emergence of the space and the energy balance relation. Here we investigate the thermodynamic properties of the universe described by such a model. We show that the first law of thermodynamics and the generalized second law of thermodynamics (GSLT) are both satisfied and the weak energy condition are also fulfilled for two typical examples. Finally we examine the physical consistency for the present model.Comment: 9 pages, 2 figure

    bβ†’cτνb\to c\tau\nu Transitions in the Standard Model Effective Field Theory

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    The R(D(βˆ—))R(D^{(\ast)}) anomalies observed in Bβ†’D(βˆ—)τνB\to D^{(\ast)}\tau\nu decays have attracted much attention in recent years. In this paper, we study the Bβ†’D(βˆ—)τνB\to D^{(\ast)}\tau\nu, Ξ›bβ†’Ξ›cτν\Lambda_b\to\Lambda_c\tau\nu, Bcβ†’(J/ψ, ηc)τνB_c\to (J/\psi,\,\eta_c)\tau\nu, Bβ†’XcτνB\to X_c\tau\nu, and Bc→τνB_c\to\tau\nu decays, all being mediated by the same quark-level bβ†’cτνb\to c\tau\nu transition, in the Standard Model Effective Field Theory. The most relevant dimension-six operators for these processes are Qlq(3)Q_{lq}^{(3)}, QledqQ_{ledq}, Qlequ(1)Q^{(1)}_{lequ}, and Qlequ(3)Q^{(3)}_{lequ} in the Warsaw basis. Evolution of the corresponding Wilson coefficients from the new physics scale Ξ›=1\Lambda=1~TeV down to the characteristic scale ΞΌb≃mb\mu_b\simeq m_b is performed at three-loop in QCD and one-loop in EW/QED. It is found that, after taking into account the constraint B(Bc→τν)≲10%{\cal B}(B_c\to\tau\nu)\lesssim 10\%, a single [Clq(3)]3323(Ξ›)\left[C_{lq}^{(3)}\right]_{3323}(\Lambda) or [Clequ(3)]3332(Ξ›)\left[C^{(3)}_{lequ}\right]_{3332}(\Lambda) can still be used to resolve the R(D(βˆ—))R(D^{(\ast)}) anomalies at 1Οƒ1\sigma, while a single [Clequ(1)]3332(Ξ›)\left[C^{(1)}_{lequ}\right]_{3332}(\Lambda) is already ruled out by the measured R(D(βˆ—))R(D^{(\ast)}) at more than 3Οƒ3\sigma. By minimizing the Ο‡2(Ci)\chi^2(C_i) function constructed based on the current data on R(D)R(D), R(Dβˆ—)R(D^\ast), PΟ„(Dβˆ—)P_\tau(D^\ast), R(J/ψ)R(J/\psi), and R(Xc)R(X_c), we obtain eleven most trustworthy scenarios, each of which can provide a good explanation of the R(D(βˆ—))R(D^{(\ast)}) anomalies at 1Οƒ1\sigma. To further discriminate these different scenarios, we predict thirty-one observables associated with the processes considered under each NP scenario. It is found that most of the scenarios can be differentiated from each other by using these observables and their correlations.Comment: 43 pages, 3 figures and 5 tables; references updated and more discussions added, final version to be published in the journa

    Revisiting the BB-physics anomalies in RR-parity violating MSSM

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    In recent years, several deviations from the Standard Model predictions in semileptonic decays of BB-meson might suggest the existence of new physics which would break the lepton-flavour universality. In this work, we have explored the possibility of using muon sneutrinos and right-handed sbottoms to solve these BB-physics anomalies simultaneously in RR-parity violating minimal supersymmetric standard model. We find that the photonic penguin induced by exchanging sneutrino can provide sizable lepton flavour universal contribution due to the existence of logarithmic enhancement for the first time. This prompts us to use the two-parameter scenario (C9V, C9U)(C^{\rm V}_9, \, C^{\rm U}_9) to explain bβ†’sβ„“+β„“βˆ’b \to s \ell^+ \ell^- anomaly. Finally, the numerical analyses show that the muon sneutrinos and right-handed sbottoms can explain bβ†’sβ„“+β„“βˆ’b \to s \ell^+ \ell^- and R(D(βˆ—))R(D^{(\ast)}) anomalies simultaneously, and satisfy the constraints of other related processes, such as Bβ†’K(βˆ—)Ξ½Ξ½Λ‰B \to K^{(\ast)} \nu \bar\nu decays, Bsβˆ’BΛ‰sB_s-\bar B_s mixing, ZZ decays, as well as D0β†’ΞΌ+ΞΌβˆ’D^0 \to \mu^+ \mu^-, τ→μρ0\tau \to \mu \rho^0, B→τνB \to \tau \nu, Ds→τνD_s \to \tau \nu, Ο„β†’KΞ½\tau \to K \nu, Ο„β†’ΞΌΞ³\tau \to \mu \gamma, and Ο„β†’ΞΌΞΌΞΌ\tau \to \mu\mu\mu decays.Comment: 10 pages, 8 figures, matches to the version published in EPJ
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