D_{sJ}(2860) as the first radial excitation of the D_{s0}^*(2317)

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Plain LaTeX, 4 pages, 2 Postscript figures; v2: REVTeX, 4 pages, introduction expanded, "Note added in proof" and references a

Scientific paper

10.1103/PhysRevLett.97.202001

A coupled-channel model previously employed to describe the narrow $D_{s0}^*$(2317) and broad $D_0^*$(2400) charmed scalar mesons is generalized so as to include all ground-state pseudoscalar-pseudoscalar and vector-vector two-meson channels. All parameters are chosen fixed at published values, except for the overall coupling constant, which is fine-tuned to reproduce the $D_{s0}^*$(2317) mass. Thus, the radial excitations $D_{s0}^*$(2850) and $D_0^*$(2740) are predicted, both with a width of about 50 MeV. The former state appears to correspond to the new $D_{sJ}$(2860) resonance decaying to $DK$ announced by BABAR in the course of this work. Also the $D_0^*$(2400) resonance is roughly reproduced, though perhaps with a somewhat too low central resonance peak.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

D_{sJ}(2860) as the first radial excitation of the D_{s0}^*(2317) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with D_{sJ}(2860) as the first radial excitation of the D_{s0}^*(2317), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and D_{sJ}(2860) as the first radial excitation of the D_{s0}^*(2317) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-409880

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.