Logo del repository
  1. Home
 
Opzioni

Angular analysis of the decay B0 to K*0 mu mu from pp collisions at sqrt(s) = 8 TeV

BELFORTE S.
•
CANDELISE, VIERI
•
CASARSA M.
altro
ZANETTI A.
2016
  • journal article

Periodico
PHYSICS LETTERS. SECTION B
Abstract
The angular distributions and the differential branching fraction of the decay B0→K⁎(892)0μ+μ−B0→K⁎(892)0μ+μ− are studied using data corresponding to an integrated luminosity of 20.5 fb−1 collected with the CMS detector at the LHC in pp collisions at View the MathML sources=8 TeV. From 1430 signal decays, the forward–backward asymmetry of the muons, the K⁎(892)0K⁎(892)0 longitudinal polarization fraction, and the differential branching fraction are determined as a function of the dimuon invariant mass squared. The measurements are among the most precise to date and are in good agreement with standard model predictions.
DOI
10.1016/j.physletb.2015.12.020
WOS
WOS:000368783600060
Archivio
http://hdl.handle.net/11368/2864209
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85040825548
http://www.sciencedirect.com/science/article/pii/S0370269315009685
Diritti
open access
license:creative commons
license uri:http://creativecommons.org/licenses/by/3.0/it/
FVG url
https://arts.units.it/bitstream/11368/2864209/2/1-s2.0-S0370269315009685-main.pdf
Soggetti
  • PARTICLE PHYSICS

  • LARGE HADRON COLLIDER...

  • CMS

Web of Science© citazioni
137
Data di acquisizione
Mar 24, 2024
google-scholar
Get Involved!
  • Source Code
  • Documentation
  • Slack Channel
Make it your own

DSpace-CRIS can be extensively configured to meet your needs. Decide which information need to be collected and available with fine-grained security. Start updating the theme to match your nstitution's web identity.

Need professional help?

The original creators of DSpace-CRIS at 4Science can take your project to the next level, get in touch!

Realizzato con Software DSpace-CRIS - Estensione mantenuta e ottimizzata da 4Science

  • Impostazioni dei cookie
  • Informativa sulla privacy
  • Accordo con l'utente finale
  • Invia il tuo Feedback