AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
  StellarModelling, Page 1 of 2  ELOG logo
ID Date Author Subject
  32   Sun Mar 17 12:11:37 2024 Selin Ezgi BirincioglumyGOE.f Nuclei
  31   Fri Mar 15 10:14:12 2024 Selin Ezgi BirinciogluNew MACS
  30   Mon Mar 11 16:29:08 2024 Selin Ezgi BirinciogluMixed Nuclei
  29   Mon Feb 19 21:42:39 2024 Selin Ezgi BirinciogluMACS

Excel Sheet of results, orange ones are nuclei that required both TALYS and mygoe.f. This file is colour coded - can be seen below the table.

  28   Sat Feb 17 21:30:23 2024 Selin Ezgi BirinciogluK43+n Variations By Combination of Models

K43-13 and -42.

  27   Sat Feb 17 20:42:03 2024 Selin Ezgi BirinciogluAr37+n Variations By Combination of Models

Ar37-13 and -42.

  26   Sat Feb 17 20:35:21 2024 Selin Ezgi BirinciogluCl36+n Variations By Combination of Models

Cl36-10 and -42.

  25   Sat Feb 17 20:18:15 2024 Selin Ezgi BirinciogluCa45+n Variations By Combination of Models

Ca45-20 and -42.

  24   Thu Feb 1 10:10:04 2024 Selin Ezgi BirinciogluList of Nuclei with MACS

This is the Excel sheet with the list of nuclei and their corresponding MACS. Yellow fill shows the nuclei with experimental cross sections, green fill shows the nuclei that obey the statistical calculations and blue fill shows the nuclei with the Gaussian distributions.

  22   Tue Jan 30 10:37:56 2024 Selin Ezgi BirinciogluK43+n Variations By Different Models

The variations of MACS distribution of K43+nwith different level density models. K43+n cannot be predicted by the statistical model below 0.025 MeV.

  21   Thu Jan 18 17:36:32 2024 Selin Ezgi BirinciogluCa45+n Variations By Different Models

The variations of MACS distribution of Ca45+n with different level density models. Ca45+n cannot be predicted by the statistical model below approx. 0.020 MeV.

  20   Thu Jan 18 15:43:13 2024 Selin Ezgi BirinciogluK41+n Variations By Different Models

The variations of MACS distribution of K41+nwith different level density models. K41+n cannot be predicted by the statistical model below 0.022 MeV.

  19   Thu Jan 18 11:08:23 2024 Selin Ezgi BirinciogluK39+n Variations By Different Models

The variations of MACS distribution of K39+nwith different level density models. K39+ncannot be predicted by the statistical model below 0.028 MeV.

  18   Thu Jan 18 10:52:48 2024 Selin Ezgi BirinciogluAr37+n Variations by Different Models

The variations of MACS distribution of Ar37+n with different level density models. Ar37+n cannot be predicted by the statistical model below 0.022 MeV.

  17   Wed Jan 17 16:15:49 2024 Selin Ezgi BirinciogluCl36+n Variations by Different Models

The variations of MACS distribution of Cl36+n with different level density models. Cl36+n cannot be predicted by the statistical model below approx. 0.020 MeV.

  16   Wed Jan 17 15:58:40 2024 Selin Ezgi BirinciogluCl35+n Variations by Different Models

The variations of MACS distribution of Cl35+n with different level density models. Cl35+n cannot be predicted by the statistical model belowe 0.026 MeV.

  15   Wed Jan 17 09:23:28 2024 Selin Ezgi BirinciogluP31+n Variations By Different Models

The variations of MACS distribution of P31+n with different nuclear models generated by TALYS.

  14   Wed Jan 17 09:17:57 2024 Selin Ezgi BirinciogluCa42+n Variations By Different Models

The variations of MACS distribution of Ca42+n with different nuclear models generated by TALYS. When the level density is high enough, the resonances seem to decrease as TALYS obeys the statistical model.

  13   Thu Nov 30 13:54:25 2023 Selin Ezgi BirinciogluFiles for Na23+n

1 -> macs.root: MACS distribution file

2 -> read.C: file to graph the histogram

3 -> list.dat: reads every run done by mygoe.f

4 -> talys.input: TALYS inputs

5 -> talys.output: output parameters for mygoe.f

6 -> Na24run: to run mygoe.f for Na23+n parameters taken from TALYS

  12   Wed Nov 8 15:20:17 2023 Selin Ezgi BirinciogluTALYS Parameters from Different Models

This is the parameters of Ca42+n and Ca50+n acquired from differen models. They were chosen as they have Gaussian distributions which are consistent with TALYS calculations of MACS. Ca42+n has experimental values while Ca50+n does not.

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