Relevant bibliographies by topics / Gamow-Teller transition

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  1. Journal articles
  2. Dissertations / Theses
  3. Book chapters
  4. Conference papers

Academic literature on the topic 'Gamow-Teller transition'

Author: Grafiati
Published: 4 June 2021
Last updated: 10 February 2022

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Journal articles on the topic "Gamow-Teller transition"

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Auerbach, Naftali, and Minh-Loc Bui. "Study of the double Gamow-Teller transitions using the shell model approach." EPJ Web of Conferences 194 (2018): 02003. http://dx.doi.org/10.1051/epjconf/201819402003.

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The double Gamow-Teller strength distributions in the lightest double beta-decay candidate 48Ca and its isotope 46Ca were calculated using the nuclear shell model by applying the single Gamow-Teller operator two times sequentially on the ground state of parent nucleus. The nuclear matrix element of the double Gamow- Teller transition from the ground state to the ground state that goes into the double beta decay calculation was shown as a small fraction of the total transition.
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QI, C., and F. R. XU. "ISOSPIN SYMMETRY AND GAMOW TELLER TRANSITION STRENGTHS IN MIRROR NUCLEI." International Journal of Modern Physics E 15, no. 07 (October 2006): 1563–68. http://dx.doi.org/10.1142/s0218301306005149.

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We have calculated the strength functions of the Gamow-Teller transition processes from mirror pairs 46 Ti –46 Cr and 50 Cr –50 Fe to the odd-odd N = Z nuclei 46 V and 50 Mn . The calculations are carried out in fp model space with shell model diagonalization method. Calculations are compared with experimental observations. We have also discussed the effects of isospin symmetry breaking on the analogous transitions.
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Obaid, S. M., and H. M. Tawfeek. "Gamow-Teller strengths of some sd-shell nuclei in the shell model framework." Revista Mexicana de Física 66, no. 3 May-Jun (May 1, 2020): 330. http://dx.doi.org/10.31349/revmexfis.66.330.

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The nuclear Gamow-Teller (GT) transition strength distributions B(GT)have been studied for some sd-shell nuclei in the (3He, t) charge-exchangereactions. The shell model calculations were performed by employing theUSDA and USDB effective interactions in the sd-model space. The results of B(GT) calculations reproduce the the experimental Gamow-Tellerstrength distributions well, while the calculated distribution of summedGT transition strengths were closely reproduce the observed ones.
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Kumar, V., P. C. Srivastava, and A. Kumar. "Gamow–Teller Transition Strengths for Selected \({fp}\) Shell Nuclei." Acta Physica Polonica B 51, no. 4 (2020): 961. http://dx.doi.org/10.5506/aphyspolb.51.961.

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Bloom, S. D., G. J. Mathews, and J. A. Becker. "Gamow–Teller strength function for 90Zr(n,p)90Y." Canadian Journal of Physics 65, no. 6 (June 1, 1987): 684–86. http://dx.doi.org/10.1139/p87-098.

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The Gamow–Teller (GT) strength function for90Zr → 90Y has been calculated in a model space including two-particle two-hole excitations from the 2p shell to the 1g9/2 shell. Our purpose here is to eventually compare this with the latest results from the 90Zr(n,p)90Y TRIUMF experiment at 0°, which should be available soon. Our calculations (as a function of the amount of ground-state correlations) predict rather similar shapes and regions of excitation but grossly different magnitudes for the total GT strength. In the case of 90Zr → 90Y, the GT transition is forbidden in zero order. Therefore, ground-state correlations must be well understood before the degree and sources for Gamow–Teller quenching can be known.
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Suzuki, Toshio, Takashi Yoshida, Michio Honma, Hélène Mao, Takaharu Otsuka, and Toshitaka Kajino. "Gamow-Teller and First-Forbidden Transition Strengths in Astrophysical Processes." Journal of Physics: Conference Series 312, no. 4 (September 23, 2011): 042023. http://dx.doi.org/10.1088/1742-6596/312/4/042023.

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Suzuki, Toshio, and Takaharu Otsuka. "Configuration of the two-neutron halo ofLi11and Gamow-Teller transition." Physical Review C 50, no. 2 (August 1, 1994): R555—R558. http://dx.doi.org/10.1103/physrevc.50.r555.

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Simpson, J. J. "Half-life of tritium and the Gamow-Teller transition rate." Physical Review C 35, no. 2 (February 1, 1987): 752–54. http://dx.doi.org/10.1103/physrevc.35.752.

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KURASAWA, HARUKI, and TOSHIO SUZUKI. "GAMOW–TELLER SUM RULE IN RELATIVISTIC NUCLEAR MODELS." Modern Physics Letters A 21, no. 12 (April 20, 2006): 935–46. http://dx.doi.org/10.1142/s0217732306020391.

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Relativistic corrections are investigated to the Gamow–Teller (GT) sum rule with respect to the difference between the β- and β+ transition strengths in nuclei. Since the sum rule requires the complete set of the nuclear states, the relativistic corrections come from the anti-nucleon degrees of freedom. In the relativistic mean field approximation, the total GT strengths carried by the nucleon sector is quenched by about 12% in nuclear matter, while by about 8% in finite nuclei, compared to the sum rule value. The coupling between the particle-hole states with the nucleon–antinucleon states is also discussed with the relativistic random phase approximation, where the divergence of the response function is renormalized with use of the counterterms in the Lagrangian. It is shown that the approximation to neglect the divergence, like the no-sea approximation extensively used so far, is unphysical, from the sum-rule point of view.
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Win, Kalayar, Yoshitaka Fujita, Yee Yeeoo, and Hiro Fujita. "Analysis of high energy resolution data of 26Mg(3He,t)26Al reaction." EPJ Web of Conferences 206 (2019): 08003. http://dx.doi.org/10.1051/epjconf/201920608003.

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The Gamow-Teller (GT) transition is a powerful tool to study nuclear structure because of its simple form of the operator στ. The structure of 26Al is studied through Gamow-Teller transitions using nuclear charge-exchange reaction. The reaction 26Mg(3He,t)26Al was performed at an incident energy of 140 MeV/nucleon and scattering angle at and near 0˚. The energy resolution of ΔE = 22 keV allowed us to study many discrete states. Most of the prominent states are suggested that they are excited with ΔL = 0 GT transitions. The GT states were studied up to 18.5 MeV. For the extraction of the B(GT) value, the proportionality between cross section and B(GT) was used. The standard B(GT) values were obtained from the 26Si beta decay, where the mirror symmetry of B(GT) was obtained. The T = 2 GT states are expected in the region Ex ≥ 13.5 MeV. By comparing with the results of 26Mg(t, 3He)26Na reactions, the isospin symmetry of T = 2 GT states is discussed. Due to the high-energy resolution, the decay widths Γ for the states in the Ex > 9 MeV region could be studied. The narrow width of the T = 2 states at 13.592 MeV is explained in terms of isospin selection rules.
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Dissertations / Theses on the topic "Gamow-Teller transition"

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Morita, Hiroyuki. "Gamow-Teller transitions in the light N = Z odd-odd nuclei:Proton-neutron correlation and SU(4) symmetry with clusters." Kyoto University, 2019. http://hdl.handle.net/2433/242608.

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Book chapters on the topic "Gamow-Teller transition"

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Bloom, Stewart D. "On the Prevalence of the Gamow-Teller Transition." In Energy in Physics, War and Peace, 15–37. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3031-5_3.

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Conference papers on the topic "Gamow-Teller transition"

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Ichikawa, Y., T. K. Onishi, D. Suzuki, H. Iwasaki, T. Kubo, V. Naik, A. Chakrabarti, et al. "Gamow-Teller transition of the proton-rich nucleus [sup 24]Si." In NUCLEAR PHYSICS TRENDS: 7th Japan-China Joint Nuclear Physics Symposium. AIP, 2010. http://dx.doi.org/10.1063/1.3442606.

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Fujita, Y., and B. Rubio. "High Resolution Charge Exchange Reaction and Analogous β-decay for the Study of Gamow-Teller Transition Strengths." In Proceedings of the 17th International Spin Physics Symposium. AIP, 2007. http://dx.doi.org/10.1063/1.2750900.

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Popescu, L. "Study of Gamow-Teller Transition Strengths in fp-shell Nuclei Using the 64Ni(d,2He)64Co Reaction." In NUCLEAR PHYSICS, LARGE AND SMALL: International Conference on Microscopic Studies of Collective Phenomena. AIP, 2004. http://dx.doi.org/10.1063/1.1805957.

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Shimbara, Y., Y. Fujita, T. Adachi, G. P. A. Berg, B. A. Brown, H. Fujimura, H. Fujita, et al. "High-resolution study of [sup 37]Cl→[sup 37]Ar Gamow-Teller transition via [sup 37]Cl([sup 3]He, t)[sup 37]Ar reaction." In THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG—2010. AIP, 2010. http://dx.doi.org/10.1063/1.3485135.

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Sasano, M., G. Perdikakis, R. G. T. Zegers, Sam M. Austin, D. Bazin, B. A. Brown, C. Caesar, et al. "Gamow-Teller transitions from [sup 56]Ni." In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011. AIP, 2012. http://dx.doi.org/10.1063/1.4763384.

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Sasano, M., H. Sakai, K. Yako, K. Miki, S. Noji, T. Wakasa, M. Dozono, et al. "Measurements of the [sup 116]Cd(p,n) and [sup 116]Sn(n,p) reactions at 300 MeV for studying Gamow-Teller transition strengths in the intermediate nucleus of the [sup 116]Cd double-β decay." In WORKSHOP ON CIRCULATION OF DOUBLE-BETA-DECAY MATRIX. AIP, 2009. http://dx.doi.org/10.1063/1.3266084.

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Nagashimaa, M., Y. Shimbara, H. Fujita, Y. Fujita, T. Adachi, N. T. Botha, E. Ganioğlu, et al. "High-resolution study of [sup 56]Fe→[sup 56]Mn Gamow-Teller transition by the combined analysis of [sup 56]Fe([sup 3]He, t)[sup 56]Co and 56Fe(P, pʹ)[sup 56]Fe reactions." In THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG—2010. AIP, 2010. http://dx.doi.org/10.1063/1.3485189.

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Fujita, Y., B. Rubio, W. Gelletly, Ismail Boztosun, and A. B. Balantekin. "Gamow-Teller Transitions in Stable and Unstable pf-shell Nuclei." In NUCLEAR PHYSICS AND ASTROPHYSICS: Nuclear Physics and Astrophysics: From Stable Beams to Exotic Nuclei. AIP, 2008. http://dx.doi.org/10.1063/1.3039861.

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Fujita, Yoshitaka. "Gamow-Teller Transitions Starting from Stable and Unstable pf-shell Nuclei." In 10th Symposium on Nuclei in the Cosmos. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.053.0018.

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Fujita, Y., T. Adachi, B. Blank, P. von Brentano, G. P. A. Berg, H. Fujita, K. Fujita, et al. "Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions." In THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG—2010. AIP, 2010. http://dx.doi.org/10.1063/1.3485193.

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