improving systematic predictions of -delayed neutron emission probabilities

15
Improving systematic predictions of - delayed neutron emission probabilities E. A. McCutchan A.A. Sonzogni T.D. Johnson NNDC D. Abriola IAEA M. Birch, B. Singh McMaster

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E. A. McCutchan A.A. Sonzogni T.D. Johnson NNDC D. Abriola IAEA M. Birch, B. Singh McMaster . Improving systematic predictions of -delayed neutron emission probabilities. Beta-delayed neutron emission. . What is it ?. P n : - PowerPoint PPT Presentation

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Page 1: Improving systematic predictions of             -delayed neutron emission probabilities

Improving systematic predictions of -delayed neutron emission probabilities

E. A. McCutchanA.A. SonzogniT.D. Johnson

NNDC

D. AbriolaIAEA

M. Birch, B. SinghMcMaster

Page 2: Improving systematic predictions of             -delayed neutron emission probabilities

Beta-delayed neutron emission

AZ+1

Q

AZ

Sn

A-1Z+1

Qn

n

What is it ? Pn : the probability to emit a

neutron following decay

Page 3: Improving systematic predictions of             -delayed neutron emission probabilities

214 nuclei with measured Pn values

http://www.nndc.bnl.gov/nudat2

Beta-delayed neutron emissionWhere is it ?

Page 4: Improving systematic predictions of             -delayed neutron emission probabilities

Beta-delayed neutron emissionWhy do we care?

• Reactor control and post-processing of fuel

• r-process nucleosynthesis and abundances

• Basic structure physics

Page 5: Improving systematic predictions of             -delayed neutron emission probabilities

5

Kratz -Herrmann Formula (KHF)

𝑃𝑛≈𝑎 [𝑄 𝛽−𝑆𝑛

𝑄𝛽−𝐶 ]𝑏

Cut off parameter C (MeV)

𝐶=0𝐶=

13√𝐴

𝐶=26√𝐴

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 linewith slope=b

Page 6: Improving systematic predictions of             -delayed neutron emission probabilities

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

Page 7: Improving systematic predictions of             -delayed neutron emission probabilities

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)

Page 8: Improving systematic predictions of             -delayed neutron emission probabilities

A better parameterization?Strength function Fermi integral

𝑃𝑛

𝑇1 /2𝑎(𝑄 𝛽𝑛)

𝑏

Applying same concept as KHF

Page 9: Improving systematic predictions of             -delayed neutron emission probabilities

With this approach

a = 0.0097(9)b = 4.87(7)red 2 = 35

a = 119(42)b = 5.45(48)red 2 = 146

Page 10: Improving systematic predictions of             -delayed neutron emission probabilities

A surprising correlation

a = 45(6)b = 4.4(4)

red 2 = 280

a = 0.037(9)b = 4.11(9)red 2 = 87

Page 11: Improving systematic predictions of             -delayed neutron emission probabilities

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, 055802 (2003).

Page 12: Improving systematic predictions of             -delayed neutron emission probabilities

Summary• New prescription for systematics of Pn values

• Ratio of Pn to T1/2

• More compact trajectory

• Seems to work across nuclear chart

Page 13: Improving systematic predictions of             -delayed neutron emission probabilities

Relevance to ENSDF

• Some evaluators give Pfeiffer KHF results (2002Pf04) for cases where Pn has not been measured

• Should we replace with values from new systematics ?

Page 14: Improving systematic predictions of             -delayed neutron emission probabilities

Another surprising correlation

P. Moller et al., Phys. Rev. C 67, 055802 (2003).

Page 15: Improving systematic predictions of             -delayed neutron emission probabilities