Search results for "Proper time"

showing 3 items of 13 documents

Measurement of the and B− meson lifetimes

1993

Abstract The lifetimes of the B 0 and B − mesons have been measured with the ALEPH detector at LEP. Semileptonic decays of B 0 and B − mesons were partially reconstructed by identifying events containing a lepton with an associated D ∗+ or D 0 meson. The proper time of the B meson was estimated from the measured decay length and the momentum and mass of the D -lepton system. A fit to the proper time of 77 D ∗+ l − and 77 D 0 l − candidates, combined with a constraint on the lifetime ratio ( τ − τ 0 ) arising from the relative rates of observed D ∗+ l − and D 0 l − events, yielded the following lifetimes: τ 0 =1.52 −0.18 +0.20 ( stat. ) −0.13 +0.07 ( syst. ) ps , τ − = 1.47 −0.19 +0.22 ( sta…

Semileptonic decayPhysicsNuclear and High Energy PhysicsParticle physicsMeson010308 nuclear & particles physicsElectron–positron annihilationNuclear TheoryHigh Energy Physics::Phenomenology01 natural sciencesNuclear physicsMomentum0103 physical sciencesDecay lengthProper timeHigh Energy Physics::ExperimentB mesonNuclear Experiment010306 general physicsLepton
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A quantum model of Schwarzschild black hole evaporation

1996

We construct a one-loop effective metric describing the evaporation phase of a Schwarzschild black hole in a spherically symmetric null-dust model. This is achieved by quantising the Vaidya solution and by chosing a time dependent quantum state. This state describes a black hole which is initially in thermal equilibrium and then the equilibrium is switched off, so that the black hole starts to evaporate, shrinking to a zero radius in a finite proper time. The naked singularity appears, and the Hawking flux diverges at the end-point. However, a static metric can be imposed in the future of the end-point. Although this end-state metric cannot be determined within our construction, we show tha…

Thermal equilibriumPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNaked singularityFOS: Physical sciencesRadiusGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum stateQuantum mechanicsMetric (mathematics)Schwarzschild metricAstronomiaProper time
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A Numbers-Based Approach to a Free Particle's Spacetime

2020

A possibility is proposed to define the proper spacetime of a free nonzerorest- mass m_0 particle based on the connection of its lasting proper time to an open sequence of natural numbers counting de Broglie time periods (h/c^2)(m^(-1)_ 0 ) [see R. Ferber, A Missing Link: What is Behind de Broglie's" Periodic Phenomenon"?, Foundations of Physics Letters 9, 575 (1996)]. It is suggested to define a set of twodirectional intervals of the particle's proper space (proper distances) following the construction of positive and negative integers from the ordered pairs of the natural numbers, which belong to the sequence 1, 2, ..., n defining the elapsed interval of de Broglie time t_n. Corresponding…

de Broglie proper timeproper spaceproper spacetime:NATURAL SCIENCES::Physics [Research Subject Categories]proper timeconstruction of integersenergy of proper space
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