1999
DOI: 10.1103/physrevlett.82.691
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Incompressibility of Nuclear Matter from the Giant Monopole Resonance

Abstract: E0 strength distributions in 90 Zr, 116 Sn, 144 Sm, and 208 Pb have been measured with inelastic scattering of 240-MeV a particles between 0 ± # u lab # 6 ± to greater precision than previously available. In Sn, Sm, and Pb, E0 strength was concentrated in approximately symmetric peaks, whereas in 90 Zr it had a significant high energy tail. Comparing with microscopic calculations using the Gogny interaction, these and our previously reported results for 40 Ca are consistent with a nuclear matter incompressibil… Show more

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Cited by 376 publications
(484 citation statements)
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“…Recent experimental data are available for the isoscalar giant monopole resonance in 116 Sn [35]. The solid curve represents the full RRPA strength and it displays a pronounced peak at 16 MeV, in excellent agreement with the measured value of 15.9 MeV [35]. Giant monopole resonances in spherical nuclei are in best agreement with experimental data, when calculated with effective Lagrangians with a nuclear matter compression modulus in the range 250-270 MeV [17,28,29].…”
Section: An Illustrative Case: the Giant Monopole Resonancesupporting
confidence: 75%
“…Recent experimental data are available for the isoscalar giant monopole resonance in 116 Sn [35]. The solid curve represents the full RRPA strength and it displays a pronounced peak at 16 MeV, in excellent agreement with the measured value of 15.9 MeV [35]. Giant monopole resonances in spherical nuclei are in best agreement with experimental data, when calculated with effective Lagrangians with a nuclear matter compression modulus in the range 250-270 MeV [17,28,29].…”
Section: An Illustrative Case: the Giant Monopole Resonancesupporting
confidence: 75%
“…3 the temperatures corresponding to the plateau regions decrease with increasing source mass, an effect that is attributed to the source temperature having reached the Coulomb instability limit [15]. From these systematics it was possible to derive a value of the critical temperature for infinite nuclear matter of 16 ± 1 MeV and a nuclear compressibility constant of K = 232 ± 30 MeV [16] in good agreement with the Giant Monopole Resonance value of K = 230 ± 5 MeV [17].…”
Section: Thermodynamics: the Caloric Curve And Heat Capacitysupporting
confidence: 65%
“…One should note, however, that the scaling calculation provides a prediction for the mean value or centroid of the excitation energy of the resonance. To establish a relation between the incompressibility K ∞ and the experimentally measured energies of the monopole mode the most favourable situation is met in heavy nuclei, where the strength of the GMR is less fragmented than in medium and light nuclei [42,49]. If we take into account the excitation energies of 116 Sn, 144 Sm and 208 Pb, according to Table 1 Refs.…”
Section: Numerical Resultsmentioning
confidence: 99%