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Phi decay: a relevant source for K- production at SIS energies?

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arxiv 0902.3487 v1 pith:7DDOE6GT submitted 2009-02-20 nucl-ex

Phi decay: a relevant source for K- production at SIS energies?

The HADES Collaboration: G.Agakishiev , A.Balanda , B.Bannier , R.Bassini , D.Belver , A.V.Belyaev , A.Blanco , M.Boehmer
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J.L.Boyard P.Braun-Munzinger P.Cabanelas E.Castro S.Chernenko T.Christ M.Destefanis J.Diaz F.Dohrmann A.Dybczak T.Eberl W.Enghardt L.Fabbietti O.V.Fateev P.Finocchiaro P.Fonte J.Friese I.Froehlich T.Galatyuk J.A.Garzon R.Gernhaeuser A.Gil1 C.Gilardi M.Golubeva D.Gonzalez-Diaz F.Guber M.Heilmann T.Heinz T.Hennino R.Holzmann A.Ierusalimov I.Iori A.Ivashkin M.Jurkovic B.Kaempfer K.Kanaki T.Karavicheva D.Kirschner I.Koenig W.Koenig B.W.Kolb R.Kotte F.Krizek R.Kruecken W.Kuehn A.Kugler A.Kurepin S.Lang J.S.Lange K.Lapidus T.Liu L.Lopes M.Lorenz L.Maier A.Mangiarotti J.Markert V.Metag B.Michalska J.Michel D.Mishra E.Moriniere J.Mousa C.Muentz L.Naumann J.Otwinowski Y.C.Pachmayer M.Palka Y.Parpottas V.Pechenov O.Pechenova T.PerezCavalcanti J.Pietraszko W.Przygoda B.Ramstein A.Reshetin M.Roy-Stephan A.Rustamov A.Sadovsky B.Sailer P.Salabura A.Schmah E.Schwab Yu.G.Sobolev S.Spataro B.Spruck H.Stroebele J.Stroth C.Sturm M.Sudol A.Tarantola K.Teilab P.Tlusty M.Traxler R.Trebac H.Tsertos V.Wagner M.Weber M.Wisniowski T.Wojcik J.Wuestenfel S.Yurevich Y.V.Zanevsky P.Zhou P.Zumbruch
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keywords decaymesonsagevbeamcomingdistributionsenergiesenergy
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We present phase space distributions and multiplicities of K+, K- and phi mesons produced in Ar+KCl reactions at a kinetic beam energy of 1.756 AGeV and measured with the HADES spectrometer. The inverse slope parameters and yields of kaons supplement the systematics of previous measurements. The percentage of K- mesons coming fromphi decay is found to be 18+- 7%.

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  1. Observation of Strong $\phi$-meson Directed Flow at High Baryon Density

    nucl-ex 2026-06 unverdicted novelty 8.0

    First observation of phi-meson directed flow v1 comparable in magnitude to protons and Lambdas but much larger than K0S, with baryon-like energy dependence at high baryon density.