143,660 research outputs found

    Measurement of surface potential decay of corona-charged polymer films using the pulsed electroacoustic method

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    In this paper, the pulsed electroacoustic (PEA) technique that allows the determination of space charge in a dielectric material has been used to monitor the electrical potential decay of corona-charged polyethylene films of different thicknesses. To prevent possible disturbance on the surface charge during the PEA measurements, two thin polyethylene films were placed on both sides of the corona-charged sample. Charge profiles measured at different times were used to calculate the potential across the sample. The obtained potential decay was compared with the potential measured using the conventional method. A good agreement has been obtained. More importantly, the charge profile obtained using the PEA technique indicates that bipolar charge injection has taken place

    Octupole degree of freedom for the critical-point candidate nucleus 152^{152}Sm in a reflection-asymmetric relativistic mean-field approach

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    The potential energy surfaces of even-even 146156^{146-156}Sm are investigated in the constrained reflection-asymmetric relativistic mean-field approach with parameter set PK1. It is shown that the critical-point candidate nucleus 152^{152}Sm marks the shape/phase transition not only from U(5) to SU(3) symmetry, but also from the octupole-deformed ground state in 150^{150}Sm to the quadrupole-deformed ground state in 154^{154}Sm. By including the octupole degree of freedom, an energy gap near the Fermi surface for single-particle levels in 152^{152}Sm with β2=0.140.26\beta_2 = 0.14 \sim 0.26 is found, and the important role of the octupole deformation driving pair ν2f7/2\nu 2f_{7/2} and ν1i13/2\nu 1i_{13/2} is demonstrated.Comment: 11 pages, 3 figure

    Discussion on Event Horizon and Quantum Ergosphere of Evaporating Black Holes in a Tunnelling Framework

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    In this paper, with the Parikh-Wilczek tunnelling framework the positions of the event horizon of the Vaidya black hole and the Vaidya-Bonner black hole are calculated respectively. We find that the event horizon and the apparent horizon of these two black holes correspond respectively to the two turning points of the Hawking radiation tunnelling barrier. That is, the quantum ergosphere coincides with the tunnelling barrier. Our calculation also implies that the Hawking radiation comes from the apparent horizon.Comment: 8 page
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