The Elasticity of the Neutron Star Mantle: The Improved Compressible Liquid Drop Model for Cylindrical Phases by Nikita A. Zemlyakov, Andrey I. Chugunov

“…In this paper, we reconsider the transverse shear modulus for cylindrical phases of the mantle within the framework of the compressible liquid drop model. We demonstrate that transverse shearing affects the shape of nuclear clusters: their cross-section becomes elliptical. …”
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Droplet model of atomic nuclei/ by 428495 Myers, William D.

Subjects: “…Nuclear liquid drop model…”

Derivation of a new formula for calculating the two neutrons' separation energy (S2n) based on the liquid-drop model by S.M. Al-Rawashdeh

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Symmetry Energy in the Inner Crust Region of Neutron Stars: A Study Around the Neutron Drip Density Point using the Compressed Liquid Drop Model by Eko Tri Sulistyani, Yusuf Panji Wisnuaji, Romy Hanang Setya Budhi

Subjects: “…symmetry energy, neutron drip, inner crust, compressible liquid drop model…”
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22.05 Neutron Science and Reactor Physics, Fall 2006 by Bernard, John A.

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1-20 MeV Enerji Aralığında 230,232Th ve 236,238,239,240,241,242,244Pu Çekirdeklerinin Nötronlarla Oluşturulan Fisyon Tesir Kesitlerinin Hesaplanması by Mustafa Yiğit, Mehmet Korkmaz, Mehtap Günay, Başar Şarer

“…In ALICE-ASH calculations, RFRM (Rotation-Finite-Range Model) and RLDM (Rotation-liquid- Drop Model) was used. The calculated fission cross section was compared with the experimental data taken from the Experimental Nuclear Reaction Data (EXFOR). …”
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Estimation of Nuclear Mass Formulas Coefficients Using Least-Squares Method Based on Gauss-Seidel Scheme: A Comparative Study Between Three Models by Hadj Mouloudj, Benyoucef Mohammed-Azizi, Oussama Zeggai, Abdelkader Ghalem, Alla Eddine Toubal Maamar

“…The obtained r.m.s. result for the new liquid drop model in terms of masses is equal to 1.05 MeV. …”
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Statistical learnability of nuclear masses by A. Idini

“…After more than 80 years from the seminal work of Weizsäcker and the liquid drop model of the atomic nucleus, deviations from experiments of mass models (∼MeV) are orders of magnitude larger than experimental errors (≲keV). …”
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Calculation of the Cluster Emission Half-Lives by Considering the Deformations and Relative Orientations of the Nuclei by P Nazarzadeh, R Bagheri

“…The calculated results are in good agreement with the experimental data and the results of the Liquid Drop Model, LDM. It is seen that with increasing the angle of the relative orientation, the systems under consideration, will be more stable against this phenomenon.…”
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Calculation The Potential Energy Surface of The Nucleus 201 Tl By Strutinsky Method by Amir Drwish Tfiha

“…Calculations based on liquid drop model and single particle model in an axially deformed Woods-Saxon potential of the fission barrier and potential energy surface of the  nucleus. …”
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Elastic properties of nuclear pasta in a fully three-dimensional geometry by Cheng-Jun Xia, Toshiki Maruyama, Nobutoshi Yasutake, Toshitaka Tatsumi, Ying-Xun Zhang

“…For slabs, due to the negligence on the variations of their thicknesses, the analytic formulae from liquid-drop model agree qualitatively but not quantitatively with our numerical estimations. …”
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Calculation The Potential Energy Surface of The Nucleus 201 Tl By Strutinsky Method by Amir Drwish Tfiha

“…Calculations based on liquid drop model and single particle model in an axially deformed Woods-Saxon potential of the fission barrier and potential energy surface of the  nucleus. …”
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Surface Vibrations of Bubble-like Superheavy Nuclei by Şerban Mişicu

“…The shape vibrations of a superheavy nucleus with a complete (bubble) or a partially (semi-bubble) depleted density in its central region and sharp-edge inner and outer surfaces are investigated in the frame of the Liquid-Drop Model. The quadrupole oscillations of the two existing surfaces are coupled in both velocity and coordinate and, upon decoupling, a low-energy and a high-energy component are predicted. …”
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Investigation of Nuclear Binding Energy and Charge Radius Based on Random Forest Algorithm by CAI Boshuai;YU Tianjun;LIN Xuan;ZHANG Jilong;WANG Zhixuan;YUAN Cenxi

“…RMSE for nuclides with Z, N>7 is reduced to 0.816 MeV and 0.020 0 fm compared with the six-term liquid drop model and a three-term nuclear charge radius formula, respectively. …”
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Formation and dissociation processes of gas-phase detergent micelles. by Borysik, A, Robinson, C

“…This relationship contradicts the thermodynamics of micelle formation in solution. However, the liquid drop model, which considers both the surface energy and charge, correlates extremely well with the experimental cluster size. …”

Transition quadrupole moments in superdeformed bands by Buck, B, Merchant, A, Perez, S

“…The choice is based on the mismatch between measured binding energies and the underlying trend supplied by the liquid drop model. A key point is that the charge to mass ratios of parent, core, and cluster should be as nearly equal as possible. …”

Skyrme interaction and nuclear matter constraints by Dutra, M, Lourenço, O, Sá Martins, J, Delfino, A, Stone, JR, Stevenson, P

“…This paper presents a detailed assessment of the ability of the 240 Skyrme interaction parameter sets in the literature to satisfy a series of criteria derived from macroscopic properties of nuclear matter in the vicinity of nuclear saturation density at zero temperature and their density dependence, derived by the liquid-drop model, in experiments with giant resonances and heavy-ion collisions. …”

From neutron skins and neutron matter to the neutron star crust by William G. Newton, Rebecca Preston, Lauren Balliet, Michael Ross

“…Using a compressible liquid drop model with an extended Skyrme energy-density functional, we obtain the most stringent constraints to date on the transition pressure Pcc=0.33−0.07+0.07 MeV fm−3 and chemical potential μcc=12.6−1.9+1,8 MeV (which control the mass, moment of inertia and thickness of a neutron star crust), the proton fractions that bracket the pasta phases yp=0.115−0.017+0.016 and ycc=0.041−0.006+0.007, as well as the relative mass and moment of inertia ΔMp/ΔMc≈ΔIp/ΔIc=0.54−0.09+0.05 and thickness ΔRp/ΔRc=0.129−0.030+0.019 of the layers of non-spherical nuclei (nuclear pasta) in the crust.…”
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Pasta Phases in Neutron Star Mantle: Extended Thomas–Fermi vs. Compressible Liquid Drop Approaches by Nikolai N. Shchechilin, Nikita A. Zemlyakov, Andrey I. Chugunov, Mikhail E. Gusakov

“…In this paper, we compare results obtained by the Extended Thomas–Fermi (ETF) method with the compressible liquid drop model (CLDM), based on the thermodynamically consistent description of the surface properties calculated for the two-phase plane interface and the same energy-density functional (for numerical illustration, we applied the Skyrme-type functional SLy4). …”
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h-BN Modification Using Several Hydroxylation and Grafting Methods and Their Incorporation into a PMMA/PA6 Polymer Blend by Abdelwahab Boukheit, France Chabert, Belkacem Otazaghine, Aurélie Taguet

“…The calculation of the wetting parameter based on the surface tension measurement using the liquid drop model showed that h-BN dispersed in the PA6 phase. …”
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