5,231 research outputs found

    Dynamical symmetries of the Klein-Gordon equation

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    The dynamical symmetries of the two-dimensional Klein-Gordon equations with equal scalar and vector potentials (ESVP) are studied. The dynamical symmetries are considered in the plane and the sphere respectively. The generators of the SO(3) group corresponding to the Coulomb potential, and the SU(2) group corresponding to the harmonic oscillator potential are derived. Moreover, the generators in the sphere construct the Higgs algebra. With the help of the Casimir operators, the energy levels of the Klein-Gordon systems are yielded naturally.Comment: 4

    Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology

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    We investigate the impacts of the gravitational-wave (GW) standard siren observation of the Einstein Telescope (ET) on constraining the total neutrino mass. We simulate 1000 GW events that would be observed by the ET in its 10-year observation by taking the standard Ξ›\LambdaCDM cosmology as a fiducial model. We combine the simulated GW data with other cosmological observations including cosmic microwave background (CMB), baryon acoustic oscillations (BAO), and type Ia supernovae (SN). We consider three mass hierarchy cases for the neutrino mass, i.e., normal hierarchy (NH), inverted hierarchy (IH), and degenerate hierarchy (DH). Using Planck+BAO+SN, we obtain βˆ‘mΞ½<0.175\sum m_\nu<0.175 eV for the NH case, βˆ‘mΞ½<0.200\sum m_\nu<0.200 eV for the IH case, and βˆ‘mΞ½<0.136\sum m_\nu<0.136 eV for the DH case. After considering the GW data, i.e., using Planck+BAO+SN+GW, the constraint results become βˆ‘mΞ½<0.151\sum m_\nu<0.151 eV for the NH case, βˆ‘mΞ½<0.185\sum m_\nu<0.185 eV for the IH case, and βˆ‘mΞ½<0.122\sum m_\nu<0.122 eV for the DH case. We find that the GW data can help reduce the upper limits of βˆ‘mΞ½\sum m_\nu by 13.7%, 7.5%, and 10.3% for the NH, IH, and DH cases, respectively. In addition, we find that the GW data can also help break the degeneracies between βˆ‘mΞ½\sum m_{\nu} and other parameters. We show that the GW data of the ET could greatly improve the constraint accuracies of cosmological parameters.Comment: 8 pages, 4 figure

    Forward Attention in Sequence-to-sequence Acoustic Modelling for Speech Synthesis

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    This paper proposes a forward attention method for the sequenceto- sequence acoustic modeling of speech synthesis. This method is motivated by the nature of the monotonic alignment from phone sequences to acoustic sequences. Only the alignment paths that satisfy the monotonic condition are taken into consideration at each decoder timestep. The modified attention probabilities at each timestep are computed recursively using a forward algorithm. A transition agent for forward attention is further proposed, which helps the attention mechanism to make decisions whether to move forward or stay at each decoder timestep. Experimental results show that the proposed forward attention method achieves faster convergence speed and higher stability than the baseline attention method. Besides, the method of forward attention with transition agent can also help improve the naturalness of synthetic speech and control the speed of synthetic speech effectively.Comment: 5 pages, 3 figures, 2 tables. Published in IEEE International Conference on Acoustics, Speech and Signal Processing 2018 (ICASSP2018
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