Parity Radius Experiment (PReX)

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Liquid/Solid Transition Density<br />

• RPA stability against<br />

small amplitude density<br />

osc. Unstable if ε L

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Liquid/Solid Transition Density • RPA stability against small amplitude density osc. Unstable if ε L

Observables Sensitive to Crust • Glitches in rotational period of pulsars from “starquakes” in solid crust. Vela crust must contain at least 1.4% of angular momentum. Crust can’t be too thin (ρ c or R can’t be too small). • Thermal properties depend on heat conduction through crust. • Solid crust can support nonaxial quadrupole deformations important for gravitational radiation. LIGO will look for signal at frequencies of known pulsars. • ...

Page 1 and 2: Parity Radius Experiment 208 Pb (PR
Page 3 and 4: Neutron Rich Skin • A heavy nucle
Page 5 and 6: Jefferson Lab Hall A exp. • 850 M
Page 7: R-process process nucleosynthesis
Page 11: Parity Radius Measurement • Provi

Parity Radius Experiment (PReX)

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