Measurement of the D*(2010)⁺ Natural Linewidth and the D*(2010)⁺—D⁰ Mass Difference
dc.contributor.VIAF | 250674117 (Izen, JM) | en_US |
dc.contributor.VIAF | 250674117 (Izen, JM) | |
dc.contributor.author | Lees, J. P. | en_US |
dc.contributor.author | Poireau, V. | en_US |
dc.contributor.author | Tisserand, V. | en_US |
dc.contributor.author | Grauges, E. | en_US |
dc.contributor.author | Palano, A. | en_US |
dc.contributor.author | Eigen, G. | en_US |
dc.contributor.author | Stugu, B. | en_US |
dc.contributor.author | Lou, Xinchou | en_US |
dc.contributor.author | Izen, Joseph M. | en_US |
dc.contributor.author | BaBar Collaboration | en_US |
dc.contributor.utdAuthor | Lou, Xinchou | en_US |
dc.contributor.utdAuthor | Izen, Joseph M. | en_US |
dc.date.accessioned | 2014-08-01T21:21:07Z | |
dc.date.available | 2014-08-01T21:21:07Z | |
dc.date.created | 2013-09-09 | en_US |
dc.date.issued | 2013-09-09 | en_US |
dc.date.submitted | 2013-04-20 | en_US |
dc.description.abstract | We measure the mass difference, Δm₀, between the D *(2010)⁺ and the D⁰ and the natural linewidth, Γ, of the transition D*(2010)⁺ → D⁰π⁺. The data were recorded with the BABAR detector at center-of-mass energies at and near the ϒ(4S) resonance, and correspond to an integrated luminosity of approximately 477 fb⁻¹. The D⁰ is reconstructed in the decay modes D⁰ → K⁻ π⁺ and D⁰ → K⁻ π⁺ π⁻ π⁺. For the decay mode D⁰ → K⁻ π⁺ we obtain Γ = (83.4 ± 1.7 ± 1.5) keV and Δm₀ = (145425.6 ± 0.6 ± 1.8) keV, where the quoted errors are statistical and systematic, respectively. For the D⁰ → K⁻ π⁺ π⁻ π⁺ mode we obtain Γ = (83.2 ± 1.5 ± 2.6) keV and Δm₀ = (145426.6 ± 0.5 ± 2.0) keV. The combined measurements yield Γ = (83.3 ± 1.2 ± 1.4) keV and Δm₀ = (145425.9 ± 0.4 ± 1.7) keV; the width is a factor of approximately 12 times more precise than the previous value, while the mass difference is a factor of approximately 6 times more precise. | en_US |
dc.identifier.bibliographicCitation | Lees, J. P., V. Poireau, V. Tisserand, E. Grauges, et al. 2013. "Measurement of the D*(2010)⁺ natural linewidth and the D*(2010)⁺—D⁰ mass difference." Physical Review D 88(5), doi:10.1103/PhysRevD.88.052003 | en_US |
dc.identifier.issn | 1550-7998 | en_US |
dc.identifier.issue | 520035 | en_US |
dc.identifier.uri | http://hdl.handle.net/10735.1/3846 | |
dc.identifier.volume | 88 | en_US |
dc.language.iso | en_US | en_US |
dc.publisher | American Physical Society | en_US |
dc.relation.uri | http://dx.doi.org/10.1103/PhysRevD..88.052003 | |
dc.rights | CC BY 3.0 (Attribution) | en_US |
dc.rights | ©2014 CERN, for the ATLAS Collaboration | en_US |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/ | en_US |
dc.source | Physical Review D - Particles, Fields, Gravitation and Cosmology | |
dc.subject | Gigaelectronvolts (GeV) | en_US |
dc.subject | Azimuthal angle | en_US |
dc.subject | Resolution functions | en_US |
dc.subject | Resolution bandwidth | en_US |
dc.subject | D0 experiment | en_US |
dc.title | Measurement of the D*(2010)⁺ Natural Linewidth and the D*(2010)⁺—D⁰ Mass Difference | en_US |
dc.type | Text | en_US |
dc.type.genre | Article | en_US |
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