A new approach to estimating the probability for  delayed neutron emission E. A. McCutchan A.A. Sonzogni T.D. Johnson National Nuclear Data Center Brookhaven.

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A new approach to estimating the probability for  delayed neutron emission E. A. McCutchan A.A. Sonzogni T.D. Johnson National Nuclear Data Center Brookhaven National Laboratory, NY USA

Outline Motivation Traditional systematics A new parameterization A closer look

 -delayed neutrons and their use Reactor control and post-processing of fuel r-process nucleosynthesis and abundances Basic structure physics

214 nuclei with measured P n values Relevance of reliable systematics

Some terminology A Z+1 QQ AZAZ SnSn A-1 Z+1 QnQn  n P n : the probability to emit a neutron following  decay

6 Kratz -Herrmann Formula (KHF) Cut off parameter C (MeV) even-even even-odd odd-odd Traditional systematic studies K.-L. Kratz and G. Herrmann, Z. Phys. A 263, 435 (1973) Two parameter fit with ‘a’ and ‘b’ Log-log plot gives straight line with slope=b

B. Pfeiffer et al., Prog. Nucl. Energy 41, 39 (2002). The standard for systematic studies Linear regression Weighted least-squares a = 106(38) b = 5.5(6) red  2 = 81

a = 119(42) b = 5.45(48) red  2 = 146 Audi and Meng (2011) Effect of improved Q values a = 106(38) b = 5.5(6) red  2 = 81 Masses from : Audi and Wapstra (1995)

A better parameterization? Strength function Fermi integral Applying same concept as KHF

A more compact trajectory a = (9) b = 4.87(7) red  2 = 35 a = 119(42) b = 5.45(48) red  2 = 146 Light fission fragment region

Heavy fission fragment region a = 141(48) b = 5.08(37) red  2 = 78 a = 0.016(2) b = 4.55(13) red  2 = 55 A more compact trajectory

A surprising correlation a = 45(6) b = 4.4(4) red  2 = 280 a = 0.037(9) b = 4.11(9) red  2 = 87 Light nuclei, Z <26

A closer look Light fission fragment region Very linear trend Few outliers 100 Rb 102 Rb

A closer look Heavy fission fragment region Few outliers Less linear trend Possible shell effects?

How do we do ?? KHF-2002: B. Pfeiffer et al., Prog. Nucl. Energy 41, 39 (2002). QRPA-1: P. Moller et al., Phys. Rev. C 67, (2003).

Another surprising correlation P. Moller et al., Phys. Rev. C 67, (2003).

Summary New prescription for systematics of P n values Ratio of P n to T 1/2 More compact trajectory Works across nuclear chart For the future Extract information about strength function from slope ??

Relevance to ENSDF Some evaluators give Pfeiffer KHF results (2002Pf04) for cases where P n has not been measured Should we replace with values from new systematics ?

Another surprising correlation P. Moller et al., Phys. Rev. C 67, (2003).