scholarly journals Number-conserving random phase approximation with analytically integrated matrix elements

1990 ◽  
Vol 41 (1) ◽  
pp. 284-297 ◽  
Author(s):  
M. Kyotoku ◽  
K. W. Schmid ◽  
F. Grümmer ◽  
Amand Faessler
2020 ◽  
Vol 9 ◽  
pp. 1
Author(s):  
Zhongzhu Ren ◽  
A. Faessler ◽  
T. S. Kosmas

The neutrinoless muon-to-electron conversion in nuclei is studied by using the renormalized quasiparticle random-phase approximation (RQRPA). This generalization of RPA is more reliable for the extremely small (μ-,e-) transition matrix elements than the ordinary QRPA because it restores the Pauli principle to a large extent. We apply the method to a set of nuclei throughout the periodic table, but we specifically investigate the 48Ti and 208Pb nuclei which are currently used as stopping targets at the PSI μ-e conversion experiments with the SINDRUM II spectrometer.


Open Physics ◽  
2014 ◽  
Vol 12 (11) ◽  
Author(s):  
Abdullah Çalık

AbstractIn the present work, the matrix elements, isospin impurities and log ft values of the isospin forbidden 0+ → 0+ beta decays have been investigated. The calculated results have been compared with available experimental and another theoretical data. The isotopic invariance of the Hamiltonian has been restored by Pyatov method. Within the quasi-particle random phase approximation (QRPA), the computations have been performed both in presence and absence of the pairing interactions.


2009 ◽  
Vol 64 (12) ◽  
pp. 865-871 ◽  
Author(s):  
Abdullah Engin Çalık ◽  
Murat Gerçeklioğlu ◽  
Djevad Irfan Salamov

In this work, the unitarity of the Cabibbo-Kobayashi-Maskawa (CKM) mixing matrix has been investigated by studying the eleven well-known superallowed Fermi Beta decays; their parent nuclei are 10C, 14O, 26Al, 34Cl, 38K, 42Sc, 46V, 50Mn, 54Co, 62Ga, and 74Rb. The numerical value of the Vud element of the CKM mixing matrix has been calculated following the standart procedure. Using a different method from those of the previous studies, the effect of the isospin breaking due to the Coulomb forces has been evaluated more accurately. Here, the shell model has been modified by Pyatov’s restoration because of the isospin breaking and the transition matrix elements have been found by means of the random phase approximation (RPA)


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