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000039452 0247_ $$2DOI$$a10.1103/PhysRevLett.83.682
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000039452 084__ $$2WoS$$aPhysics, Multidisciplinary
000039452 1001_ $$0P:(DE-Juel1)VDB39762$$aSewerin, S. H.$$b0$$uFZJ
000039452 245__ $$aComparison of lambda and sigma (0) production near threshold in proton-proton collisions
000039452 260__ $$aCollege Park, Md.$$bAPS$$c1999
000039452 300__ $$a682
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000039452 440_0 $$04925$$aPhysical Review Letters$$v83$$x0031-9007$$y4
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000039452 520__ $$aThreshold measurements of the associated strangeness production reactions pp --> pK(+)Lambda and pp --> pK(+)Sigma(0) are presented. The most remarkable feature of the data is that at the same excess energy the total cross section for the Sigma(0) production appears to be about a factor of 28(-9)(+6) smaller than for the Lambda particle. It is concluded that strong Sigma(0)p final state interactions, and in particular the Sigma N --> Lambda p conversion reaction, are the likely cause of the depletion in the Sigma signal. This hypothesis is in line with other experimental evidence in the literature.
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000039452 7001_ $$0P:(DE-Juel1)VDB1406$$aSchepers, G.$$b1$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aBalewski, J. T.$$b2
000039452 7001_ $$0P:(DE-HGF)0$$aBudzanowski, A.$$b3
000039452 7001_ $$0P:(DE-HGF)0$$aEyrich, W.$$b4
000039452 7001_ $$0P:(DE-HGF)0$$aFritsch, M.$$b5
000039452 7001_ $$0P:(DE-HGF)0$$aGoodman, C.$$b6
000039452 7001_ $$0P:(DE-Juel1)VDB513$$aGrzonka, D.$$b7$$uFZJ
000039452 7001_ $$0P:(DE-Juel1)131179$$aHaidenbauer, J.$$b8$$uFZJ
000039452 7001_ $$0P:(DE-Juel1)131182$$aHanhart, C.$$b9$$uFZJ
000039452 7001_ $$0P:(DE-Juel1)VDB7007$$aHofmann, M.$$b10$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aJarczyk, L.$$b11
000039452 7001_ $$0P:(DE-Juel1)VDB20197$$aJochmann, M.$$b12$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aKhoukaz, A.$$b13
000039452 7001_ $$0P:(DE-Juel1)VDB749$$aKilian, K.$$b14$$uFZJ
000039452 7001_ $$0P:(DE-Juel1)VDB18057$$aKöhler, M.$$b15$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aLister, T.$$b16
000039452 7001_ $$0P:(DE-HGF)0$$aMoskal, P.$$b17
000039452 7001_ $$0P:(DE-Juel1)VDB1182$$aOelert, W.$$b18$$uFZJ
000039452 7001_ $$0P:(DE-Juel1)VDB39763$$aPellmann, I.$$b19$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aQuentmeier, C.$$b20
000039452 7001_ $$0P:(DE-HGF)0$$aSanto, R.$$b21
000039452 7001_ $$0P:(DE-HGF)0$$aSeddik, U.$$b22
000039452 7001_ $$0P:(DE-Juel1)131326$$aSefzick, T.$$b23$$uFZJ
000039452 7001_ $$0P:(DE-HGF)0$$aStinzing, F.$$b24
000039452 7001_ $$0P:(DE-HGF)0$$aStrzalkowski, A.$$b25
000039452 7001_ $$0P:(DE-HGF)0$$aWilkin, C.$$b26
000039452 7001_ $$0P:(DE-Juel1)VDB1804$$aWolke, M.$$b27$$uFZJ
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000039452 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.83.682$$gVol. 83, p. 682$$p682$$q83<682$$tPhysical review letters$$v83$$x0031-9007$$y1999
000039452 8567_ $$uhttp://dx.doi.org/10.1103/PhysRevLett.83.682
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