Results 1 to 10 of about 764,047 (274)
Complete factorization in minimal N=4 $$ \mathcal{N}=4 $$ Chern-Simons-matter theory
We investigate an N=4UNk×UN+M−k $$ \mathcal{N} = 4\;\mathrm{U}{(N)}_k\times \mathrm{U}{\left(N+M\right)}_{-k} $$ Chern-Simons theory coupled to one bifundamental hypermultiplet by employing its partition function, which is given by 2N + M dimensional ...
Tomoki Nosaka, Shuichi Yokoyama
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Congruences modulo prime for fractional colour partition function [PDF]
Purpose – Let p[1,r;t] be defined by ∑n=0∞p[1,r;t](n)qn=(E1Er)t, where t is a non-zero rational number, r ≥ 1 is an integer and Er=∏n=0∞(1−qr(n+1)) for |q|
Riyajur Rahman, Nipen Saikia
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Calculation of the Free Energy of the Ising Model on a Cayley Tree via the Self-Similarity Method
In this study, an interactive Ising model having the nearest and prolonged next-nearest neighbors defined on a Cayley tree is considered. Inspired by the results obtained for the one-dimensional Ising model, we will construct the partition function and ...
Hasan Akın
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By employing the extended Nikiforov–Uvarov (ENU) method, we solved the radial Schrodinger equation with the shifted screened Kratzer potential model.
Nuhu Ibrahim +4 more
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We discuss integrable aspects of the logarithmic contribution of the partition function of cosmological critical topologically massive gravity. On one hand, written in terms of Bell polynomials which describe the statistics of set partitions, the ...
Yannick Mvondo-She
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The vibrational and rovibrational partition functions of diatomic molecules are considered in the regime of intermediate temperatures. The low temperatures are those at which the harmonic oscillator approximation is appropriate, and the high temperatures
Marcin Buchowiecki
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Context. Hydrogen is the most abundant molecule in the Universe. Its thermodynamic quantities dominate the physical conditions in molecular clouds, protoplanetary disks, etc. It is also of high interest in plasma physics. Therefore thermodynamic data for molecular hydrogen have to be as accurate as possible in a wide temperature range.Aims.
Popovas, Andrius, Jørgensen, Uffe Gråe
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Classical Partition Function for Non-Relativistic Gravity
We considered the canonical gravitational partition function Z associated to the classical Boltzmann–Gibbs (BG) distribution e−βHZ. It is popularly thought that it cannot be built up because the integral involved in constructing Z diverges at the origin.
Mir Hameeda +3 more
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Matrix string partition functions [PDF]
harvmac (b), 15 pages.
Kostov, Ivan K., Vanhove, Pierre
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Gluing Nekrasov Partition Functions [PDF]
37 pages, references added, typos ...
Qiu, Jian +3 more
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