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Probing the Symmetry Energy with the Spectral Pion Ratio

(SπRIT Collaboration) Estee, J; Lynch, WG; Tsang, CY; Barney, J; Jhang, G; Tsang, MB; Wang, R; Kaneko, M; Lee, JW; Isobe, T et al. [Show all]; Kurata-Nishimura, M; Murakami, T; Ahn, DS; Atar, L; Aumann, T; Baba, H; Boretzky, K; Brzychczyk, J; Cerizza, G; Chiga, N; Fukuda, N; Gasparic, ; Hong, B; Horvat, A; Ieki, K; Inabe, N; Kim, YJ; Kobayashi, T; Kondo, Y; Lasko, P; Lee, HS; Leifels, Y; Lukasik, J; Manfredi, J; McIntosh, AB; Morfouace, P; Nakamura, T; Nakatsuka, N; Nishimura, S; Otsu, H; Pawlowski, P; Pelczar, K; Rossi, D; Sakurai, H; Santamaria, C; Sato, H; Scheit, H; Shane, R; Shimizu, Y; Simon, H; Snoch, A; Sochocka, A; Sumikama, T; Suzuki, H; Suzuki, D; Takeda, H; Tangwancharoen, S; Toernqvist, H; Togano, Y; Xiao, ZG; Yennello, SJ; Zhang, Y; Cozma, MD. [Show fewer] (2021) Probing the Symmetry Energy with the Spectral Pion Ratio. Physical Review Letters, 126 (16). ISSN 0031-9007

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Abstract

Many neutron star properties, such as the proton fraction, reflect the symmetry energy contributions to the equation of state that dominate when neutron and proton densities differ strongly. To constrain these contributions at suprasaturation densities, we measure the spectra of charged pions produced by colliding rare isotope tin (Sn) beams with isotopically enriched Sn targets. Using ratios of the charged pion spectra measured at high transverse momenta, we deduce the slope of the symmetry energy to be 42 < L < 117 MeV. This value is slightly lower but consistent with the L values deduced from a recent measurement of the neutron skin thickness of Pb-208.

Item Type: Article
Uncontrolled Keywords: Nuclear equation of states; symmetry energy; heavy-ion collisions; pions
Subjects: NATURAL SCIENCES > Physics
Divisions: Division of Experimental Physics
Projects:
Project titleProject leaderProject codeProject type
Zemljovid atomskih jezgara - neutronski bogata strana-NeRiS-LandSuzana SzilnerIP-2018-01-1257HRZZ
Nuklearna struktura i reakcije: eksperimentima prema neutronskoj liniji kapanja-SR-ETNoSuzana SzilnerIP-2013-11-7194HRZZ
Depositing User: Lorena Palameta
Date Deposited: 29 Apr 2025 07:25
URI: http://fulir.irb.hr/id/eprint/9769
DOI: 10.1103/physrevlett.126.162701

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