S. R. Das Gupta
University of North Bengal
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by S. R. Das Gupta.
Astrophysics and Space Science | 1977
S. R. Das Gupta
We obtain a new representation of ChandrasekharsH-functionsH(z) corresponding to the dispersion functionT(z) = |δrs−frs(z)|, [frs(z)] is of rank one.H(z) is obtained in the formAbstractWe obtain a new representation of ChandrasekharsH-functionsH(z) corresponding to the dispersion functionT(z) = |δrs−frs(z)|, [frs(z)] is of rank one.H(z) is obtained in the form
Astrophysics and Space Science | 1974
S. R. Das Gupta
Astrophysics and Space Science | 1978
S. R. Das Gupta
H\left( z \right) = \left( {A_0 + A_1 z} \right)/\left( {K + z} \right) - \sum\limits_1^n {\int\limits_{E_r } {P_r (x) dx/(x + z),} }
Astrophysics and Space Science | 1978
S. R. Das Gupta
Astrophysics and Space Science | 1978
S. R. Das Gupta
WherePrx(=ør(x)/H(x)) is continuous onErwhich are subsets of [0, 1].Ao,A1are determinable constants andK is the positive root ofT(z),ør(x) are known functions. From this formH(z) is then obtained in terms of a Fredholm type integral equation. This new form ofH(z) has proved to be very useful in solving coupled integral equations involvingX-,Y-functions of transport problems.Pr(x) can be replaced by approximating polynomials whose coefficients can be determined as functions of the moments of known functions; a closed form approximation ofH(z) to a sufficiently high degree of accuracy is then readily available by term integrations.
Astrophysics and Space Science | 1980
S. R. Das Gupta; Z. Islam; S. K. Bishnu
ChandrasekharsH-functionH(z) corresponding to the dispersion functionT(z)=|δ rs −frs(z)|, where [f rs (z)] is of rank 1, is obtained in terms of a Cauchy integral whose density functionQ(x,ω 1,ω 2,...) can be approximated by approximating polynomials (uniformly converging toQ(x)) having their coefficients expressed as known functions of the parametersω r s. A closed form approximation ofH(z) to a sufficiently high degree of accuracy is then readily available by term by term integration.
Astrophysics and Space Science | 1987
S. K. Bishnu; S. R. Das Gupta
Some useful results and remodelled representations ofH-functions corresponding to the dispersion function
Astrophysics and Space Science | 1987
Santanu Das Gupta; S. R. Das Gupta
Astrophysics and Space Science | 1991
Santanu Das Gupta; S. R. Das Gupta
T\left( z \right) = 1 - 2z^2 \sum\limits_1^n {\int_0^{\lambda r} {Y_r } \left( x \right){\text{d}}x/\left( {z^2 - x^2 } \right)}
Astrophysics and Space Science | 1991
S. K. Bishnu; S. R. Das Gupta