Last edited by Munris
Sunday, July 26, 2020 | History

3 edition of The K̄ [symbol for pi] nucleon final state in KP interactions at 5.5 GeV/c found in the catalog.

The K̄ [symbol for pi] nucleon final state in KP interactions at 5.5 GeV/c

The K̄ [symbol for pi] nucleon final state in KP interactions at 5.5 GeV/c

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  • 21 Currently reading

Published .
Written in English


Edition Notes

Statementby Herbert Earl Schulz.
Classifications
LC ClassificationsMicrofilm 42513 (Q)
The Physical Object
FormatMicroform
Paginationvii, 109 leaves
Number of Pages109
ID Numbers
Open LibraryOL2019056M
LC Control Number90954224


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The K̄ [symbol for pi] nucleon final state in KP interactions at 5.5 GeV/c Download PDF EPUB FB2

An analysis of the final state K* found in these topologies and based on preliminary data, has already been published [ 1 ]. $ Work supported by the US Atomic Energy Commission and the National Science Foundation. ~ Now at Louisiana State University.

46 R. Davis et al., K -d interactions at GeV,1c by: 7. A variation of the model proposed by Plahte and Roberts is used to fit data from the reaction K − p → K 0 π − p at GeV/ channel K − p → K ∗− p is also studied in some detail and the energy dependence of the cross section is discussed.

The behaviour of the differential cross sections and of the density matrix elements of K ∗ in the G-J frame as function of t' suggests Cited by: 5. The total cross-section of the pp → nK+Σ+ reaction was measured at COSY using a proton beam with a momentum of p beam = GeV/c, corresponding to an excess energy of ε = MeV.

The method involves B→DK decays where the neutral D decays to the K0 Sπ+π- final state, together with the sample of decays of CP-tagged D mesons (produced, e.g. in ψ()→DD̄ process) to. Indication of a Deeply Bound and Compact K pp State Formed in the pp. p Kþ Reaction at GeV T.

Yamazaki,1,2 M. Maggiora,3 P. Kienle,4,5 K. Suzuki,4 A. Amoroso,3. Planck's law describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature T, when there is no net flow of matter or energy between the body and its environment.

At the end of the 19th century, physicists were unable to explain why the observed spectrum of black-body radiation, which by then had been accurately measured.

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