Minimal color-flavor-locked-nuclear interface
By M. Alford, Kumbakonam R. Rajagopal, S. Reddy, Frank Wilczek. 2001
148 citations recorded by the source corpus.
Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Radiation
View Paper: https://www.semanticscholar.org/paper/40819e5ec67c2343d440912651a29d27b5ffbd8d
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In Atomic and Molecular Physics, and Optics
In Nuclear and High Energy Physics
Citations in the corpus
- QUARK MATTER IN MASSIVE COMPACT STARS (2011, unknown): “We adopt the EoS from Alford et al. (2001) which introduces the pairing energy ∆ as a new free parameter: ΩCFL= 6 π2 ∫ ν 0 dp p2(p− µ) + 3 π2 ∫ ν 0 dp p2( √ p2 +m2s − µ) +(1− a4) 3µ4 4π2 − 3∆2µ2 π2 +Beff , (2) where ν = 2µ − √ µ2 −m2s/3.”
- Hybrid Stars that Masquerade as Neutron Stars (2004, methodology): “The critical surface tension is c 40 MeV fm 3 (Heiselberg et al. 1993; Alford et al. 2001b).”