The atomic nucleus is composed of two different kinds of fermions: protons and neutrons. If the protons and neutrons did not interact, the Pauli exclusion principle would force the majority of fermions (usually neutrons) to have a higher average momentum. Our high-energy electron-scattering measurements using (12)C, (27)Al, (56)Fe, and (208)Pb targets show that even in heavy, neutron-rich nuclei, short-range interactions between the fermions form correlated high-momentum neutron-proton pairs. Thus, in neutron-rich nuclei, protons have a greater probability than neutrons to have momentum greater than the Fermi momentum. This finding has implications ranging from nuclear few-body systems to neutron stars and may also be observable experimentally in two-spin-state, ultracold atomic gas systems.

Nuclear physics. Momentum sharing in imbalanced Fermi systems

LENISA, Paolo;
2014

Abstract

The atomic nucleus is composed of two different kinds of fermions: protons and neutrons. If the protons and neutrons did not interact, the Pauli exclusion principle would force the majority of fermions (usually neutrons) to have a higher average momentum. Our high-energy electron-scattering measurements using (12)C, (27)Al, (56)Fe, and (208)Pb targets show that even in heavy, neutron-rich nuclei, short-range interactions between the fermions form correlated high-momentum neutron-proton pairs. Thus, in neutron-rich nuclei, protons have a greater probability than neutrons to have momentum greater than the Fermi momentum. This finding has implications ranging from nuclear few-body systems to neutron stars and may also be observable experimentally in two-spin-state, ultracold atomic gas systems.
2014
Hen, O; Sargsian, M; Weinstein, L. B; Piasetzky, E; Hakobyan, H; Higinbotham, D. W; Braverman, M; Brooks, W. K; Gilad, S; Adhikari, K. P; Arrington, J; Asryan, G; Avakian, H; Ball, J; Baltzell, N. A; Battaglieri, M; Beck, A; May Tal Beck, S; Bedlinskiy, I; Bertozzi, W; Biselli, A; Burkert, V. D; Cao, T; Carman, D. S; Celentano, A; Chandavar, S; Colaneri, L; Cole, P. L; Crede, V; D'Angelo, A; De Vita, R; Deur, A; Djalali, C; Doughty, D; Dugger, M; Dupre, R; Egiyan, H; El Alaoui, A; El Fassi, L; Elouadrhiri, L; Fedotov, G; Fegan, S; Forest, T; Garillon, B; Garcon, M; Gevorgyan, N; Ghandilyan, Y; Gilfoyle, G. P; Girod, F. X; Goetz, J. T; Gothe, R. W; Griffioen, K. A; Guidal, M; Guo, L; Hafidi, K; Hanretty, C; Hattawy, M; Hicks, K; Holtrop, M; Hyde, C. E; Ilieva, Y; Ireland, D. G; Ishkanov, B. I; Isupov, E. L; Jiang, H; Jo, H. S; Joo, K; Keller, D; Khandaker, M; Kim, A; Kim, W; Klein, F. J; Koirala, S; Korover, I; Kuhn, S. E; Kubarovsky, V; Lenisa, Paolo; Levine, W. I; Livingston, K; Lowry, M; Lu, H. Y; Macgregor, I. J. D; Markov, N; Mayer, M; Mckinnon, B; Mineeva, T; Mokeev, V; Movsisyan, A; Munoz Camacho, C; Mustapha, B; Nadel Turonski, P; Niccolai, S; Niculescu, G; Niculescu, I; Osipenko, M; Pappalardo, L. L; Paremuzyan, R; Park, K; Pasyuk, E; Phelps, W; Pisano, S; Pogorelko, O; Price, J. W; Procureur, S; Prok, Y; Protopopescu, D; Puckett, A. J. R; Rimal, D; Ripani, M; Ritchie, B. G; Rizzo, A; Rosner, G; Roy, P; Rossi, P; Sabatié, F; Schott, D; Schumacher, R. A; Sharabian, Y. G; Smith, G. D; Shneor, R; Sokhan, D; Stepanyan, S. S; Stepanyan, S; Stoler, P; Strauch, S; Sytnik, V; Taiuti, M; Tkachenko, S; Ungaro, M; Vlassov, A. V; Voutier, E; Walford, N. K; Wei, X; Wood, M. H; Wood, S. A; Zachariou, N; Zana, L; Zhao, Z. W; Zheng, X; Zonta, I.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/2327534
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