The Batchelor–Chandrasekhar equation is the evolution equation for the scalar functions, defining the two-point velocity correlation tensor of a homogeneous axisymmetric turbulence, named after George Batchelor and Subrahmanyan Chandrasekhar.
[1][2][3][4] They developed the theory of homogeneous axisymmetric turbulence based on Howard P. Robertson's work on isotropic turbulence using an invariant principle.
[5] This equation is an extension of Kármán–Howarth equation from isotropic to axisymmetric turbulence.
The theory is based on the principle that the statistical properties are invariant for rotations about a particular direction
(say), and reflections in planes containing
This type of axisymmetry is sometimes referred to as strong axisymmetry or axisymmetry in the strong sense, opposed to weak axisymmetry, where reflections in planes perpendicular to
[6] Let the two-point correlation for homogeneous turbulence be A single scalar describes this correlation tensor in isotropic turbulence, whereas, it turns out for axisymmetric turbulence, two scalar functions are enough to uniquely specify the correlation tensor.
In fact, Batchelor was unable to express the correlation tensor in terms of two scalar functions, but ended up with four scalar functions, nevertheless, Chandrasekhar showed that it could be expressed with only two scalar functions by expressing the solenoidal axisymmetric tensor as the curl of a general axisymmetric skew tensor (reflectionally non-invariant tensor).
be the unit vector which defines the axis of symmetry of the flow, then we have two scalar variables,
represents the cosine of the angle between
be the two scalar functions that describes the correlation function, then the most general axisymmetric tensor which is solenoidal (incompressible) is given by, where The differential operators appearing in the above expressions are defined as Then the evolution equations (equivalent form of Kármán–Howarth equation) for the two scalar functions are given by where
is the kinematic viscosity and The scalar functions
are related to triply correlated tensor
are related to the two point correlated tensor
The triply correlated tensor is Here
is the density of the fluid.
During decay, if we neglect the triple correlation scalars, then the equations reduce to axially symmetric five-dimensional heat equations, Solutions to these five-dimensional heat equation was solved by Chandrasekhar.
The initial conditions can be expressed in terms of Gegenbauer polynomials (without loss of generality), where
are Gegenbauer polynomials.
The required solutions are where
is the Bessel function of the first kind.
the solutions become independent of