Spherical bessel functions jn and yn of integer order and real argument

1984 ◽  
Vol 35 ◽  
pp. C-466
Author(s):  
R.W.B. Ardill ◽  
K.J.M. Moriarty
1980 ◽  
Vol 22 (3) ◽  
pp. 431-438 ◽  
Author(s):  
F. Beukers

It is shown that a simple trick involving Legendre polynomials readily yields the irrationality of ea, , π2, and of the zeros of Bessel functions of integer order. Generalisation of this idea yields the irrationality of ζ(3).


2008 ◽  
pp. 537-552
Author(s):  
Keith B. Oldham ◽  
Jan C. Myland ◽  
Jerome Spanier

2008 ◽  
Vol 51 (4) ◽  
pp. 627-636
Author(s):  
Mirjana V. Vidanović ◽  
Slobodan B. Tričković ◽  
Miomir S. Stanković

AbstractIn this paper we derive formulas for summation of series involving J. Bourget's generalization of Bessel functions of integer order, as well as the analogous generalizations by H. M. Srivastava. These series are expressed in terms of the Riemann ζ function and Dirichlet functions η, λ, β, and can be brought into closed form in certain cases, which means that the infinite series are represented by finite sums.


2006 ◽  
Vol 15 (08) ◽  
pp. 1311-1327 ◽  
Author(s):  
S. HANSRAJ ◽  
S. D. MAHARAJ

We present solutions to the Einstein–Maxwell system of equations in spherically symmetric gravitational fields for static interior space–times with a specified form of the electric field intensity. The condition of pressure isotropy yields three category of solutions. The first category is expressible in terms of elementary functions and does not have an uncharged limit. The second category is given in terms of Bessel functions of half-integer order. These charged solutions satisfy a barotropic equation of state and contain Finch–Skea uncharged stars. The third category is obtained in terms of modified Bessel functions of half-integer order and does not have an uncharged limit. The physical features of the charged analogue of the Finch–Skea stars are studied in detail. In particular, the condition of causality is satisfied and the speed of sound does not exceed the speed of light. The physical analysis indicates that this analogue is a realistic model for static charged relativistic perfect fluid spheres.


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