Inclusive production of multistrange hyperons from 11-GeV/cK−p interactions | Zendy

D. Aston | Zendy; R.K. Carnegie | Zendy; W. Dunwoodie | Zendy; S. Durkin | Zendy; P.G. Estabrooks | Zendy; R.J. Hemingway | Zendy; A. K. Honma | Zendy; D. P. Hutchinson | Zendy; W.B. Johnson | Zendy; P. Kunz | Zendy; T. A. Lasinski | Zendy; D. W. G. S. Leith | Zendy; L. J. Levinson | Zendy; R. J. McKee | Zendy; B. Meadows | Zendy; A.C. McPherson | Zendy; W. T. Meyer | Zendy; G. Oakham | Zendy; B. N. Ratcliff | Zendy; S. Shapiro | Zendy; T. Shimomura | Zendy; S. Suzuki | Zendy; J. Va’vra | Zendy; S. Williams | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Inclusive production of multistrange hyperons from 11-GeV/cK−p interactions

Author(s) -

D. Aston,

R.K. Carnegie,

W. Dunwoodie,

S. Durkin,

P.G. Estabrooks,

R.J. Hemingway,

A. K. Honma,

D. P. Hutchinson,

W.B. Johnson,

P. Kunz,

T. A. Lasinski,

D. W. G. S. Leith,

L. J. Levinson,

R. J. McKee,

B. Meadows,

A.C. McPherson,

W. T. Meyer,

G. Oakham,

B. N. Ratcliff,

S. Shapiro,

T. Shimomura,

S. Suzuki,

J. Va’vra,

S. Williams

Publication year - 1985

Publication title -

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Language(s) - English

Resource type - Journals

eISSN - 1089-4918

pISSN - 0556-2821

DOI - 10.1103/physrevd.32.2270

Subject(s) - physics , hyperon , particle physics , production (economics) , nuclear physics , hadron , economics , macroeconomics

Large samples of inclusively produced 8-, n- and H'(l530) events are pre- sented from a 1427 ev/pb exposure of the LASS spectrometer to an 11 GeV/c K- beam. Production characteristics of these states are compared with other data and shown to be consistent with hyperon exchange. Polarization of B- shows an increase in magnitude with both Feynman x and transverse momen- tum. The H- decay parameters are measured to be are = -0.40 f 0.03 and tDPH = (5f 10)'. R es&s of searches for higher mass hyperons are presented. The E-(1820) + 8" (1530)7r- d eta y is observed, while we fail to confirm the existence of the x+(3170).

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research