Revisiting Axial-Vector Meson Mixing

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages

Scientific paper

10.1016/j.physletb.2011.12.013

Various phenomenological studies indicate that the mixing angle $\theta_{K_1}$ of $K_{1A}$ and $K_{1B}$, the strange partners of the axial-vector mesons $a_1(1260)$ and $b_1(1235)$, respectively, lies in the vicinity of $35^\circ$ or $55^\circ$, but whether this angle is larger or smaller than $45^\circ$ still remains controversial. When the $f_1(1285)$-$f_1(1420)$ mixing angle $\theta_{^3P_1}$ and the $h_1(1170)$-$h_1(1380)$ mixing angle $\theta_{^1P_1}$ are determined from the mass relations, they depend on the masses of $K_{1A}$ and $K_{1B}$, which in turn depend on the mixing angle $\theta_{K_1}$. We show that the approximate decoupling of the light $q\bar q$ state from the heavier $s \bar s$ state, which is empirically valid for vector, tensor and $3^{--}$ mesons, when applied to isoscalar axial-vector mesons, will enable us to discriminate different solutions of $\theta_{^3P_1}$ and $\theta_{^1P_1}$ and pick up $\theta_{K_1}\sim 35^\circ$. Indeed, for $\theta_{K_1}\sim 55^\circ$, the predicted $\theta_{^1P_1}$ disagrees sharply with the recent lattice calculation and the implied large $s\bar s$ content of $h_1(1170)$ and $q\bar q$ component of $h_1(1380)$ cannot explain the observation of their strong decays. We conclude that $\theta_{K_1}$ is smaller than $45^\circ$.

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

Revisiting Axial-Vector Meson Mixing 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 Revisiting Axial-Vector Meson Mixing, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Revisiting Axial-Vector Meson Mixing will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-471266

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