Detailed spectroscopy of doubly magic 
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Sn</mml:mi><mml:mprescripts /><mml:none /><mml:mn>132</mml:mn></mml:mmultiscripts></mml:math>

Benito, J.; Fraile, L. M.; Korgul, A.; Adamska, Edyta; Andreyev, A. N.; Álvarez-Rodríguez, R.; Barzakh, A. E.; Berry, T.; Borge, M. J. G.; Carmona, M.; Chrysalidis, K.; Costache, C.; Cubiss, J. G.; Goodacre, T. Day; Witte, H. De; Fedorov, D. V.; Fedosseev, V. N.; Fernández-Martínez, G.; Fijałkowska, A.; Fila, M.; Fynbo, H. O. U.; Galaviz, D.; Galve, P.; García-Díez, M.; Greenlees, P. T.; Grzywacz, R.; Harkness-Brennan, L. J.; Henrich, C.; Huýse, M.; Ibáñez, P.; Illana, A.; Janas, Z.; Jolie, J.; Judson, D. S.; Karayonchev, V.; Kicińska‐Habior, M.; Konki, J.; Kurcewicz, J.; Lazarus, I.; Lică, R.; López-Montes, A.; Lund, M. V.; Mach, H.; Madurga, M.; Marroquín, I.; Marsh, B. A.; Martínez, M.; Mazzocchi, C.; Mărginean, N.; Mărginean, R.; Miernik, K.; Mihai, C.; Mihai, R.; Nácher, E.; Negreţ, A.; Page, R. D.; Paulauskas, S. V.; Pascu, S.; Perea, Á.; Pucknell, V.; Rahkila, P.; Raison, C.; Rapisarda, E.; Régis, J.-M.; Rezynkina, K.; Rotaru, F.; Rothe, S.; Sánchez-Parcerisa, Daniel; Sánchez-Tembleque, V.; Schomacker, K.; Simpson, G. S.; Sotty, Ch.; Stan, L.; Stănoiu, M.; Stryjczyk, M.; Tengblad, O.; Turturică, A.; Udı́as, J. M.; Duppen, Piet Van; Vedia, V.; Villa-Abaunza, A.; Víñals, S.; Walters, W. B.; Wadsworth, R.; Warr, N.

doi:10.1103/physrevc.102.014328

Cited by 10 publications

(6 citation statements)

References 46 publications

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“…The crucial contribution in the wave function comes from the RPA one-phonon configuration. The results are in reasonable agreement with the experimental data [44,57,58]. It is worth mentioning that the first discussion of the PPC effect on the 2 + 1 and 3 − 1 properties calculated with Skyrme forces was published in [45].…”

Section: The Frsa Modelsupporting

confidence: 88%

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Origin of Low- and High-Energy Monopole Collectivity in 132Sn

Arsenyev

Severyukhin

2021

Universe

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Beginning with the Skyrme interaction, we study the properties of the isoscalar giant monopole resonances (ISGMR) of 132Sn. Using the finite-rank separable approximation for the particle-hole interaction, the coupling between one- and two-phonon terms in the wave functions of excited states is taken into account in very large configurational spaces. The inclusion of the phonon–phonon coupling (PPC) results in the formation of a low-energy 0+ state. The PPC inclusion leads to a fragmentation of the ISGMR strength to lower energy states and also to a higher energy tail. Using the same set of parameters, we describe the available experimental data for the ISGMR characteristics of 118,120,122,124Sn and give a prediction for 126,128,130,132Sn.

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Section: The Frsa Modelsupporting

confidence: 88%

“…The PPC effects are taken into account. The experimental data are taken from[44,57,58]. The B(Eλ; λ π 1 → 0 + gs ) values are given in Weisskopf units.…”

mentioning

confidence: 99%

Origin of Low- and High-Energy Monopole Collectivity in 132Sn

Arsenyev

Severyukhin

2021

Universe

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“…So, deviation of experimental B(E 2) from the microscopic structure calculations is observed for 4 + 1 level in both N = 80 and 84 Te, one with two valence neutron holes and the other with two valence neutron particles with respect to the 132 Sn core. It is known that most of the levels in 132 Sn core correspond to particle-hole excitations across the N = 82 shell gap [48]. The 4 + 1 level in 132 Sn is originated with one neutron particle excited across N = 82 to the νf However, the model space (jj55pna) used in the present shell model calculation considers orbitals in the 50-82 subshell space and do not include single-particle f 7 2 orbital beyond N = 82.…”

Section: Discussionmentioning

confidence: 99%

Lifetimes and transition probabilities for low-lying yrast levels in Te130,132

et al. 2022

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“…The weighted mass-excess value of two measurements for the 1 + isomer is = −83 473. 45(92) keV and the energy difference between 1 + and 8 − + 5 + states is 77.2 (15) keV.…”

Section: Inmentioning

confidence: 98%

“…Neutron-rich indium isotopes around the doubly magic 132 Sn nucleus are a center of attention and they are extensively studied via a plethora of experimental methods, such as mass measurements [1][2][3][4], laser spectroscopy [5,6], decay spectroscopy [7][8][9][10][11][12][13][14][15][16][17][18], and transfer reactions [19]. It is because nuclei around the doubly magic core are relatively simple systems and they constitute a perfect testing ground for various theoretical approaches [20][21][22][23][24][25].…”

Section: Introductionmentioning

confidence: 99%