Appendix C

Some Mathematical Relations

C.1  SOME ALGEBRAIC RELATIONS

C.1.1  Expansions

(a ± b)2 = a2 ± 2ab + b2

 

(a ± b)3 = a3 ± 3a2b + 3ab2 ± b3

 

(a ± b)4 = a4 ± 4a3 b + 6a2b2 ± 4ab3 + b4
equation

Here the binomial co-efficient equation is called ‘factorial r’.

C.1.2  Factors

a2 – b2 = (a + b)(a – b)

 

a3 ± b3 = (a ± b)(a2ab + b2)

 

an – bn = (a – b)(an – 1 + an – 2 b + ··· + bn – 1)

 

an + bn = (a + b)(an – 1 – an – 2 b + ··· + bn – 1), for n odd.

C.1.3  Sum of Numbers

equation
equation

C.1.4  Binomial Series for x2 < 1

equation
(1 ± x)–1 = 1 ∓ x + x2x3 + x4 ···

 

(1 ± x)–2 = 1 ∓ 2x + 3x2 ∓ 4x3 + 5x4 ···

C.1.5  Exponential Series

equation

C.1.6  Logarithmic Series

equation
C.2  SOME TRIGONOMETRIC RELATIONS

C.2.1  Fundamental Identities

sin2α + cos2α = 1

 

1 + tan2α = sec2α

 

1 + cot2 α = cosec2α

 

sin (α ± β) = sin α cos β ± cos α sin β

 

cos (α ± β) = cos α cos β ∓ sin α sin β
equation
sin2 α = 2sin α cos α

 

cos 2α = cos2α – sin2α = 2cos2α – 1 = 1 – 2sin2α
equation
sin3α = 3sin α – 4sin3 α

 

cos 3α = 4 cos3α – 3 cosα
equation
equation

C.2.2  Relations among Inverse Functions

equation
equation

C.2.3  Hyperbolic Functions

equation
sinh (x ± y) = sinh x cosh y ± cosh x sinh y

 

cosh(x ± y) = cosh x cosh y ± sinh x sinh y

C.2.4  Connection between Circular and Hyperbolic Functions

eix = cos x + i sin x, equation
eix = cos xi sin x
equation
tan x = − i tanh ix

C.2.5  Trigonometric Series

equation
equation
C.3  COORDINATE SYSTEMS
  1. Cartesian Coordinate System
    Figure C.1

    Figure C.1 Cartesian coordinate system. The differential volume is dV = dx dy dz

  2. Spherical Coordinate System
    equation
    equation
    Figure C.2

    Figure C.2 Spherical coordinate system. The differential volume is dV = r2 sin θ dr dθ dϕ

Unit vectors ex, ey, ez in cartesian coordinate system and er, eθ, eϕ in spherical coordinate system are related as

equation

or

equation

The components of vector A = (Ax, Ay, Az) and A = (Ar, Aθ, Aϕ) are related through the transformation

equation

or through inverse transformation

equation
C.4  SOME VECTOR RELATIONS

C.4.1  Cartesian Coordinates (x, y, z)

equation
equation
equation
equation
equation

C.4.2  Spherical Polar Coordinates (r, θ, ϕ)

equation
equation
equation
equation
equation

C.4.3  Relations Involving the ∇ Operator

Here A, B, C denote vectors; ϕ, ψ denote scalars.

 

∇(ϕ ψ) = ϕψ + ψϕ         (C. 15a)

 

∇ × (A + B) = ∇ × A + ∇ × B         (C.15b)

 

∇ · (ϕ A) = A · ∇ϕ + ϕ∇ · A         (C.15c)

 

∇ × (ϕA) = ϕ∇ × AA × ∇ϕ         (C.15d)

 

∇ · (A × B) = B · ∇ × AA · ∇ × B         (C.15e)

 

∇ × (A × B) = (B · ∇) AB∇ · A – (A · ∇) B + A∇ · B         (C.15f)

 

∇(A · B) = (B · ∇)A + (A · ∇)B + B × ∇ × A + A × ∇ × B         (C.15g)

 

∇ × ∇ × A = ∇(∇ · A) – ∇2A         (C.15h)

C.4.4  Other Vector Relations

A × (B × C) = B(A · C) – C(A · B)         (C.16a)
equation
equation

If r denotes the position vector, then

 

∇ · r = 3        (C.17a)

 

∇ × r = 0        (C.17b)

 

rn = nrn – 2r        (C.17c)

 

2rn = n(n + 1)rn – 2        (C.17d)
equation

(Gauss) Divergence Theorem: The normal surface integral of a vector function F over the boundary of a closed surface (of arbitrary shape) is equal to the volume integral of the divergence of F taken over the enclosed volume. In mathematical form it is expressed as

equation

(Stokes) Curl Theorem: If a vector function F and its first derivative are continuous, the line integral of F around a closed curve C is equal to the normal surface integral of Curl F over an open surface bounded by C. In mathematical form it is expressed as

equation
C.5  SOME CALCULUS RELATIONS

C.5.1  Derivatives

If U = U(x), V = V(x), and b = constant

equation
equation

C.5.2  Integrals

equation
equation
equation
C.6  SOME DEFINITE INTEGRALS
equation
equation
equation
equation
C.7  AN IMPORTANT INTEGRAL

If the electronic charge density in a state in an atom is ρ(r) (e.g. in s-state of an electron), which is spherically symmetric, then the self-potential energy of the charge cloud is

equation

Let us consider the work done in building up this charge distribution. In the process of built up, let us consider that a sphere of charge of radius r is already built. The potential at the surface of this sphere is

equation

Then the work done in bringing more charge from infinity to form a spherical shell of thickness dr and density ρ(r) at the surface of sphere of radius r already present,

equation

The total self-potential energy for the entire charge distribution is

equation

Let us take ρ(r) = e2αr, so

equation

Integrating by parts, the second integral gives

equation

So

equation
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