Symmetry Energy and Neutron Skins: Where do the extra neutrons go? Rskin ≡ Rn −Rp International Workshop on Nuclear Dynamics and Thermodynamics in Honor of Professor Joe Natowitz

First Page		Document Content
Date: 2013-08-26 15:10:03 Star types Baryons Nuclear technology Neutron Nuclear matter Compact star Parity Physics Nuclear physics Exotic matter		Symmetry Energy and Neutron Skins: Where do the extra neutrons go? Rskin ≡ Rn −Rp International Workshop on Nuclear Dynamics and Thermodynamics in Honor of Professor Joe Natowitz Add to Reading List Source URL: iwndt.tamu.edu Download Document from Source Website File Size: 3,76 MB Share Document on Facebook

	Hadrons baryons mesons fermions DocID: 1v7xl - View Document
	Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, ) Ξ BARYONS (S = −2, I = 1/2) Ξ 0 = uss, DocID: 1v4xM - View Document
	Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, ) ∆ BARYONS (S = 0, I = 3/2) ∆++ = u u u, DocID: 1uyHK - View Document
	Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, CHARMED BARYONS (C = +1) ++ 0 DocID: 1uoXm - View Document
	Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, BOTTOM BARYONS (B = −1) − Λ0b = u d b, Ξ 0b = u s b, Ξ − DocID: 1u7oo - View Document