Please use this identifier to cite or link to this item:
http://hdl.handle.net/10397/5397
| DC Field | Value | Language |
|---|---|---|
| dc.contributor | Department of Applied Physics | - |
| dc.creator | O'Donnell, PJ | - |
| dc.creator | Xu, QP | - |
| dc.creator | Tung, HKK | - |
| dc.date.accessioned | 2014-12-11T08:25:42Z | - |
| dc.date.available | 2014-12-11T08:25:42Z | - |
| dc.identifier.issn | 1550-7998 | - |
| dc.identifier.uri | http://hdl.handle.net/10397/5397 | - |
| dc.language.iso | en | en_US |
| dc.publisher | American Physical Society | en_US |
| dc.rights | Physical Review D © 1995 The American Physical Society. The Journal's web site is located at http://prd.aps.org/ | en_US |
| dc.subject | B mesons | en_US |
| dc.subject | Form factors (elementary particles) | en_US |
| dc.subject | Meson decay | en_US |
| dc.subject | Quark mass | en_US |
| dc.subject | Quark models | en_US |
| dc.subject | Scaling phenomena | en_US |
| dc.subject | Semileptonic decays | en_US |
| dc.subject | Weak particle decay | en_US |
| dc.title | Weak decays in the light-front quark model | en_US |
| dc.type | Journal/Magazine Article | en_US |
| dc.identifier.spage | 3966 | - |
| dc.identifier.epage | 3977 | - |
| dc.identifier.volume | 52 | - |
| dc.identifier.issue | 7 | - |
| dc.identifier.doi | 10.1103/PhysRevD.52.3966 | - |
| dcterms.abstract | We study the form factors of heavy-to-heavy and heavy-to-light weak decays using the light-front relativistic quark model. For the heavy-to-heavy B→D(*) semileptonic decays we calculate the corresponding Isgur-Wise function for the while kinematic region. For the heavy-to-light B→P and B→V semileptonic decays we calculate the form factors at q²=0; in particular, we have derived the dependence of the form factors on the b-quark mass in the mb→∞ limit. This dependence cannot be produced by extrapolating the scaling behavior of the form factors at q[sub max]² using the single-pole assumption. This shows that the q² dependence of the form factors in regions far away from the zero recoil could be much more complicated than that predicted by the single-pole assumption. | - |
| dcterms.accessRights | open access | en_US |
| dcterms.bibliographicCitation | Physical review. D, Particles, fields, gravitation, and cosmology, Oct. 1995, v. 52, no. 7, p. 3966-3977 | - |
| dcterms.isPartOf | Physical review. D, Particles, fields, gravitation, and cosmology | - |
| dcterms.issued | 1995-10-01 | - |
| dc.identifier.isi | WOS:A1995TL18200025 | - |
| dc.identifier.scopus | 2-s2.0-33751084401 | - |
| dc.identifier.eissn | 1550-2368 | - |
| dc.description.oa | Version of Record | en_US |
| dc.identifier.FolderNumber | OA_IR/PIRA | en_US |
| dc.description.pubStatus | Published | en_US |
| dc.description.oaCategory | VoR allowed | en_US |
| Appears in Collections: | Journal/Magazine Article | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| ODonnell_Decays_Light-front_Quark.pdf | 520.47 kB | Adobe PDF | View/Open |
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