A polynomial expansion for cross sections has been introduced in the 3D Method Of Characteristics (MOC) solver of the APOLLO3 code, with the aim of applying the method to depleted systems. This paper addresses the suitable adaptation of the MOC equations with regards to the free and DPN-accelerated power iterations, describing also how the conceived algorithms take advantage of a vectorized implementation. An adaptive quadrature technique is presented, necessary for the evaluation of terms that, due to the polynomial description, cannot be solved analytically. The decisive advantage of the new method over a classical step-constant description of nuclear properties is assessed by comparing the results of the depletion study of a PWR assembly.

Cross sections polynomial axial expansion within the APOLLO3 3D characteristics method / Gammicchia, A.; Santandrea, S.; Dulla, S.. - In: ANNALS OF NUCLEAR ENERGY. - ISSN 0306-4549. - 165:(2022).

Cross sections polynomial axial expansion within the APOLLO3 3D characteristics method

S. Dulla
2022

Abstract

A polynomial expansion for cross sections has been introduced in the 3D Method Of Characteristics (MOC) solver of the APOLLO3 code, with the aim of applying the method to depleted systems. This paper addresses the suitable adaptation of the MOC equations with regards to the free and DPN-accelerated power iterations, describing also how the conceived algorithms take advantage of a vectorized implementation. An adaptive quadrature technique is presented, necessary for the evaluation of terms that, due to the polynomial description, cannot be solved analytically. The decisive advantage of the new method over a classical step-constant description of nuclear properties is assessed by comparing the results of the depletion study of a PWR assembly.
2022
File in questo prodotto:
File Dimensione Formato  
1-s2.0-S0306454921005491-main.pdf

accesso riservato

Tipologia: 2a Post-print versione editoriale / Version of Record
Licenza: Non Pubblico - Accesso privato/ristretto
Dimensione 7.71 MB
Formato Adobe PDF
7.71 MB Adobe PDF   Visualizza/Apri   Richiedi una copia
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11583/2996488