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Dive into the research topics where Necla Çakmak is active.

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Featured researches published by Necla Çakmak.


Physics of Atomic Nuclei | 2012

Low-lying Gamow-Teller transitions in spherical nuclei

Necla Çakmak; Serdar Ünlü; Cevad Selam

The Pyatov Method has been used to study the low-lying Gamow-Teller transitions in the mass region of 98 ⩽ A ⩽ 130. The eigenvalues and eigenfunctions of the total Hamiltonian have been solved within the framework of proton-neutron quasiparticle random-phase approximation. The low-lying β decay log(ft) values have been calculated for the nuclei under consideration.


European Physical Journal A | 2016

First-forbidden

Jameel-Un Nabi; Necla Çakmak; Zafar Iftikhar

Abstract.First-forbidden (FF) transitions can play an important role in decreasing the calculated half-lives specially in environments where allowed Gamow-Teller (GT) transitions are unfavored. Of special mention is the case of neutron-rich nuclei where, due to phase-space amplification, FF transitions are much favored. We calculate the allowed GT transitions in various pn-QRPA models for even-even neutron-rich isotopes of nickel. Here we also study the effect of deformation on the calculated GT strengths. The FF transitions for even-even neutron-rich isotopes of nickel are calculated assuming the nuclei to be spherical. Later we take into account deformation of nuclei and calculate GT + unique FF transitions, stellar


Central European Journal of Physics | 2014

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Hasan Ali Aygör; Serdar Ünlü; Necla Çakmak; Cevat Selam

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Physica Scripta | 2015

-decay rates, energy rates of

Jameel-Un Nabi; Necla Çakmak; Sabin Stoica; Zafar Iftikhar

-decay rates, energy rate of


Turkish journal of physics | 2016

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Serdar Ünlü; Hasan Ali Aygör; Necla Çakmak; Cevad Selam

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Cumhuriyet Science Journal | 2016

-delayed neutrons and probability of

Şule Duygu; Necla Çakmak

-delayed neutrons and probability of


Pramana | 2010

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Necla Çakmak; Serdar Ünlü; Cevad Selam

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Pramana | 2010

-delayed neutron emissions for neutron-rich nickel isotopes

Necla Çakmak; Kaan Manisa; Serdar Ünlü; Cevad Selam

-delayed neutron emissions. The calculated half-lives are in excellent agreement with measured ones and might contribute in speeding-up of the r-matter flow.


Nuclear Physics | 2015

Deformation effects on isospin mixing and isobar analogue resonance for 74−80Kr isotopes

Serdar Ünlü; Necla Çakmak

Pyatov’s method has been applied to investigate Fermi beta transitions in deformed 74–80Kr isotopes. This self-consistent method, which was used to study the isobar analogue states in the spherical odd-odd nuclei, has to date not been applied for the isobar analogue states in deformed nuclei. The nucleon-nucleon residual interaction has been included so that the broken isospin symmetry in the mean field approximation has been restored and the strength parameter of the effective interaction has been taken out to be a free parameter. The energies and wave functions of the isobaric analogue excitations in 74–80Rb isotopes have been obtained within the framework of the pnQRPA method. The probability of the isospin mixing in the ground states and the centroid energies of the isobar analogue resonance have been presented and the deformation effects on these quantities have been quantified.


Nuclear Physics | 2017

First-forbidden transitions and stellar β-decay rates of Zn and Ge isotopes

Serdar Ünlü; Necla Çakmak; Cevad Selam

First-forbidden (FF) charge-changing transitions become relatively important for nuclei as their proton number increases. This is because the strength of allowed Gamow–Teller (GT) transitions decreases with increasing Z. The FF transitions play an important role in reducing the half-lives compared to those calculated from taking the GT transitions alone into account. In this paper we calculate allowed GT as well as and transitions for neutron-rich Zn and Ge isotopes. Two different pn-QRPA models were used with a schematic separable interaction to calculate GT and FF transitions. Half-lives calculated after inclusion of FF transitions were in excellent agreement with the experimental data. Our calculations were also compared to previous QRPA calculations and were found to be in better agreement with measured data. Stellar β-decay rates were calculated for these nuclei including allowed GT and unique FF transitions for astrophysical applications. 86,88Ge has a sizeable contribution to the total stellar rate from unique FF transitions.

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Serdar Ünlü

Mehmet Akif Ersoy University

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Cevad Selam

Muş Alparslan University

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Cevat Selam

Muş Alparslan University

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Sadiye Cakmak

Eskişehir Osmangazi University

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