We present the first observation of K- and φ absorption within nuclear matter by means of π - induced reactions on C and W targets at an incident beam momentum of 1.7 GeV/c studied with HADES at SIS18/GSI. The double ratio (K-/K+)W/(K-/K+)C is found to be 0.319±0.009(stat)-0.012+0.014(syst) indicating a larger absorption of K- in heavier targets as compared to lighter ones. The measured φ/K- ratios in π-+C and π-+W reactions within the HADES acceptance are found to be equal to 0.55±0.04(stat)-0.07+0.06(syst) and to 0.63±0.06(stat)-0.11+0.11(syst), respectively. The similar ratios measured in the two different reactions demonstrate for the first time experimentally that the dynamics of the φ meson in nuclear medium is strongly coupled to the K- dynamics. The large difference in the φ production off C and W nuclei is discussed in terms of a strong φN in-medium coupling. These results are relevant for the description of heavy-ion collisions and the structure of neutron stars.

Strong Absorption of Hadrons with Hidden and Open Strangeness in Nuclear Matter

Spataro S.;
2019-01-01

Abstract

We present the first observation of K- and φ absorption within nuclear matter by means of π - induced reactions on C and W targets at an incident beam momentum of 1.7 GeV/c studied with HADES at SIS18/GSI. The double ratio (K-/K+)W/(K-/K+)C is found to be 0.319±0.009(stat)-0.012+0.014(syst) indicating a larger absorption of K- in heavier targets as compared to lighter ones. The measured φ/K- ratios in π-+C and π-+W reactions within the HADES acceptance are found to be equal to 0.55±0.04(stat)-0.07+0.06(syst) and to 0.63±0.06(stat)-0.11+0.11(syst), respectively. The similar ratios measured in the two different reactions demonstrate for the first time experimentally that the dynamics of the φ meson in nuclear medium is strongly coupled to the K- dynamics. The large difference in the φ production off C and W nuclei is discussed in terms of a strong φN in-medium coupling. These results are relevant for the description of heavy-ion collisions and the structure of neutron stars.
2019
123
2
022002-1
022002-6
https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.123.022002
Adamczewski-Musch J.; Arnold O.; Atomssa E.T.; Behnke C.; Belounnas A.; Belyaev A.; Berger-Chen J.C.; Biernat J.; Blanco A.; Blume C.; Bohmer M.; Cher...espandi
File in questo prodotto:
File Dimensione Formato  
PhysRevLett.123.022002.pdf

Accesso riservato

Descrizione: Articolo originale
Tipo di file: PDF EDITORIALE
Dimensione 324 kB
Formato Adobe PDF
324 kB Adobe PDF   Visualizza/Apri   Richiedi una copia
1812.03728.pdf

Accesso aperto

Descrizione: Arxiv
Tipo di file: POSTPRINT (VERSIONE FINALE DELL’AUTORE)
Dimensione 207.21 kB
Formato Adobe PDF
207.21 kB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1804561
Citazioni
  • ???jsp.display-item.citation.pmc??? 0
  • Scopus 19
  • ???jsp.display-item.citation.isi??? 15
social impact