7,441 research outputs found

    Quantum Private Comparison: A Review

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    As an important branch of quantum secure multiparty computation, quantum private comparison (QPC) has attracted more and more attention recently. In this paper, according to the quantum implementation mechanism that these protocols used, we divide these protocols into three categories: The quantum cryptography QPC, the superdense coding QPC, and the entanglement swapping QPC. And then, a more in-depth analysis on the research progress, design idea, and substantive characteristics of corresponding QPC categories is carried out, respectively. Finally, the applications of QPC and quantum secure multi-party computation issues are discussed and, in addition, three possible research mainstream directions are pointed out

    Matter Power Spectra in Viable f(R)f(R) Gravity Models with Massive Neutrinos

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    We investigate the matter power spectra in the power law and exponential types of viable f(R)f(R) theories along with massive neutrinos. The enhancement of the matter power spectrum is found to be a generic feature in these models. In particular, we show that in the former type, such as the Starobinsky model, the spectrum is magnified much larger than the latter one, such as the exponential model. A greater scale of the total neutrino mass, Σmν\Sigma m_{\nu}, is allowed in the viable f(R)f(R) models than that in the Λ\LambdaCDM one. We obtain the constraints on the neutrino masses by using the CosmoMC package with the modified MGCAMB. Explicitly, we get $\Sigma m_{\nu} < 0.451 \ (0.214)\ \mathrm{eV}at95thecorrespondingoneforthe at 95% C.L. in the Starobinsky (exponential) model, while the corresponding one for the \LambdaCDMmodelisCDM model is \Sigma m_{\nu} < 0.200\ \mathrm{eV}.Furthermore,bytreatingtheeffectivenumberofneutrinospecies. Furthermore, by treating the effective number of neutrino species N_{\mathrm{eff}}asafreeparameteralongwith as a free parameter along with \Sigma m_{\nu},wefindthat, we find that N_{\mathrm{eff}} = 3.78^{+0.64}_{-0.84} (3.47^{+0.74}_{-0.60})and and \Sigma m_{\nu} = 0.533^{+0.254}_{-0.411}( (< 0.386) \ \mathrm{eV}$ at 95% C.L. in the Starobinsky (exponential) model.Comment: 15 pages, 5 figures, updated version accepted by PL
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