Parity – Violating Neutron Density Measurements (On Behalf of the PREX Collaboration ) Robert Michaels Concept PREX, C-REX : 208Pb Experiments Elastic electron scattering from a nucleus Flux Integration.
Download ReportTranscript Parity – Violating Neutron Density Measurements (On Behalf of the PREX Collaboration ) Robert Michaels Concept PREX, C-REX : 208Pb Experiments Elastic electron scattering from a nucleus Flux Integration.
Parity – Violating Neutron Density Measurements (On Behalf of the PREX Collaboration ) Robert Michaels Concept PREX, C-REX : 208Pb Experiments Elastic electron scattering from a nucleus Flux Integration Technique PREX: 500 MHz C-REX : 80 MHz Z0 is a Clean Probe that couples mainly to Neutrons d d 2 GF Q d R d L A 2 2 d d d R d L p, n 2 FN (Q ) 2 1 4 sin W 2 FP (Q ) HRS spectrometers target w/ Coulomb distortions (C. J. Horowitz) : proton Weak charge 208Pb of neutron Electric charge 1 0 Weak charge 0.08 1 dA 3% A dRn 1% Rn Pol. Source Hall A JLAB CEBAF Nuclear Structure: Neutron density is a fundamental observable that remains elusive. HRS spectrometers Pb target fig: C.J. Horowitz Reflects poor understanding of symmetry energy of nuclear matter = the energy cost of N Z HRS Septum Magnet Lead / diamond sandwich, cryo-cooled . 50 target E(n, x) E(n, x 1/ 2) S (n) (1 2 x ) 2 n Applications x Neutron Density Ratio Neutron / Proton Nuclear Structure fig: B. A. Brown Results, New Proposals E/N PREX-I Result PREX & Neutron Stars PRL 108 (2012) 112502 PRC 85 (2012) 03250(R) N A 0.656 ppm 0.060( stat) 0.014(syst ) C.J. Horowitz, J. Piekarewicz Asymmetry leads to RN Establishing a neutron skin at ~95 % CL RN calibrates equation of state (pressure vs density) of Neutron Rich Matter Neutron Skin = RN - RP = 0.33 + 0.16 - 0.18 fm . Low Q2 test of Standard Model . Needs H PNC Some Neutron Stars seem too cold Might be explained by cooling by neutrino emission (URCA process) depending on symmetry energy. 2 GF 2 RN theory: P. Ring , et.al 2 N N (r ) Z (1 4 sin W ) P (r ) e/ 5 e d 3 r published approved to run RN - RP Strange star ? Quark Star ? dRN 0.9 % RN (conditionally approved) Application: Atomic Parity Violation Combine PREX RN with Observed Neutron Star Radii Phase Transition to “Exotic” Core ? C-REX Proposal A