39,308 research outputs found

    Polarization amplitudes in τ−→ντVP\tau^- \to \nu_{\tau} V P decay beyond the standard model

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    We use a recent formalism of the weak hadronic reactions τ−→ντM1M2\tau^- \to \nu_{\tau} M_1 M_2 to study the helicity amplitudes in τ−→ντVP\tau^- \to \nu_{\tau} V P decay. This recent formalism maps the transition matrix elements at the quark level into hadronic matrix elements, and finally writes the weak matrix elements in terms of easy analytical formulas evaluated by means of an elaborate angular momentum algebra. The formalism provides directly the amplitudes for the different spin third components of the vector mesons involved. We extend the formalism to a general case, with the operator γμ−αγμγ5\gamma^\mu -\alpha\gamma^\mu \gamma_5, that can account for different models beyond the standard model and study in detail the τ−→ντK∗0K−\tau^- \to \nu_{\tau} K^{*0} K^{-} reaction for the different helicities of the K∗0K^{*0}. The results are shown in terms of the α\alpha parameter that differs for each model. We find that dΓdMinv(K∗0K−)\frac{d \Gamma}{d M_{\rm inv}^{(K^{*0} K^{-} )}} is very different for the different components M=±1,0M=\pm 1, 0 and in particular the magnitude dΓdMinv(K∗0K−)∣M=+1−dΓdMinv(K∗0K−)∣M=−1\frac{d \Gamma}{d M_{\rm inv}^{(K^{*0} K^{-} )}}|_{M=+1} -\frac{d \Gamma}{d M_{\rm inv}^{(K^{*0} K^{-} )}}|_{M=-1} is very sensitive to the α\alpha parameter, which makes the investigation of this magnitude a most welcome initiative to test different models beyond the standard model.Comment: 20 pages, 6 figures, add some discussion

    Helicity amplitudes in B→D∗νˉlB \to D^{*} \bar{\nu} l decay

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    We use a recent formalism of the weak hadronic reactions that maps the transition matrix elements at the quark level into hadronic matrix elements, evaluated with an elaborate angular momentum algebra that allows finally to write the weak matrix elements in terms of easy analytical formulas. In particular they appear explicitly for the different spin third components of the vector mesons involved. We extend the formalism to a general case, with the operator γμ−αγμγ5\gamma^\mu -\alpha\gamma^\mu \gamma_5, that can accommodate different models beyond the standard model and study in detail the B→D∗νˉlB \to D^{*} \bar{\nu} l reaction for the different helicities of the D∗D^*. The results are shown for each amplitude in terms of the α\alpha parameter that is different for each model. We show that dΓdMinv(νl)\frac{d \Gamma}{d M_{\rm inv}^{(\nu l)}} is very different for the different components M=±1,0M=\pm 1, 0 and in particular the magnitude dΓdMinv(νl)∣M=−1−dΓdMinv(νl)∣M=+1\frac{d \Gamma}{d M_{\rm inv}^{(\nu l)}}|_{M=-1} -\frac{d \Gamma}{d M_{\rm inv}^{(\nu l)}}|_{M=+1} is very sensitive to the α\alpha parameter, which suggest to use this magnitude to test different models beyond the standard model. We also compare our results with the standard model and find very similar results, and practically identical at the end point of Minv(νl)=mB−mD∗M_{\rm inv}^{(\nu l)}= m_B- m_{D^*}.Comment: 25 pages, 10 figure

    Three pseudoscalar meson production in e+e−e^+ e^- annihilation

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    We study, at leading order in the large number of colours expansion and within the Resonance Chiral Theory framework, the odd-intrinsic-parity e+e−→π+π−(π0,η)e^+ e^- \rightarrow \pi^+ \pi^- (\pi^0, \eta) cross-sections in the energy regime populated by hadron resonances, namely 3 \, m_{\pi} \lsim E \lsim 2 \, \mbox{GeV}. In addition we implement our results in the Monte Carlo generator PHOKHARA 7.0 and we simulate hadron production through the radiative return method.Comment: 39 pages, 5 figure

    Transport equation for 2D electron liquid under microwave radiation plus magnetic field and the Zero Resistance State

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    A general transport equation for the center of mass motion is constructed to study transports of electronic system under uniform magnetic field and microwave radiation. The equation is applied to study 2D electron system in the limit of weak disorder where negative resistance instability is observed when the radiation field is strong enough. A solution of the transport equation with spontaneous AC current is proposed to explain the experimentally observed Radiation-Induced Zero Resistance State.Comment: 9 pages, 1 figur

    B0→D0Dˉ0K0B^0 \to D^0 \bar D^0 K^0, B+→D0Dˉ0K+B^+ \to D^0 \bar D^0 K^+ and the scalar DDˉD \bar D bound state

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    We study the B0B^0 decay to D0Dˉ0K0D^0 \bar D^0 K^0 based on the chiral unitary model that generates the X(3720) resonance, and make predictions for the D0Dˉ0D^0 \bar D^0 invariant mass distribution. From the shape of the distribution, the existence of the resonance below threshold could be induced. We also predict the rate of production of the X(3720) resonance to the D0Dˉ0D^0 \bar D^0 mass distribution with no free parameters.Comment: 9 pages, 17 figure
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