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《中国物理C》(英文)编辑部
2024年10月30日

COSMIC RAY'S DATA OF MEAN LIVES OF D MESONS AND c+ BARYON

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Zhao Shu-song and Peng Shou-li. COSMIC RAY'S DATA OF MEAN LIVES OF D MESONS AND c+ BARYON[J]. Chinese Physics C, 1980, 4(4): 531-535.
Zhao Shu-song and Peng Shou-li. COSMIC RAY'S DATA OF MEAN LIVES OF D MESONS AND c+ BARYON[J]. Chinese Physics C, 1980, 4(4): 531-535. shu
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Received: 1979-06-14
Revised: 1900-01-01
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COSMIC RAY'S DATA OF MEAN LIVES OF D MESONS AND c+ BARYON

Abstract: A sieve-comparison method is proposed according to the accelerator's data ofcharmed particles to identify the properties of the X-particles observed in high energycosmic ray interactions. The principles of the sieve-comparison method are as follows: 1. The cross section σx<span style="border-top: 1px solid; padding-top: 0px;">x</span> of these X-particles produced in pair should be appro-ximately equal to the cross section σDD of D meson produced in pair. 2. The empirical selection rules of the decay in weak interaction from the experi-ments using accelerators should be suitable to these X-particles: charmed number|Δc|=1, strangeness ΔSc=1, isospin |ΔI3| =1→|ΔI|=1, (nonlepton). 3. The charge and the decay channel should be in coincidence with the empiricalselection rule, Q=I3+(B+C)/2 for each X particle and it's transverse momentumshould be large (P=400-1000MeV/c). 4. For the same kind of the particles, their width-mass ratio (г/M) should beof the same order of magnitude. All the X particles observed so far in emulsion chambers have been analyzedaccording to this method, it is found that they are possibly D, <span style="border-top: 1px solid; padding-top: 0px;">D</span>, Σc+, Λc+, Ecc+, (seetable I). Inversely, we may estimate the mean lives and masses of new charmed parti-cles observed in accelerator's experiments according to cosmic ray's data. The resultsare shown in table II.

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