﻿ The Methodology of Mathematical Particle Physics
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 The Methodology of Mathematical Particle Physics

## The Lagrangian Scheme

The most abstract version of the mechanics of systems of particles involve the formulation of the Lagrangian function for the system. Let K denote the kinetic energy of the system and V its potential energy. The Lagrangian function for a discrete system is simply the difference K−V, the difference of its kinetic and potential energy, expressed in terms of the state variables of the system and their time derivatives as well as any parameters affecting the system, such as electrical, magnetic or gravitational field intensities.

The dynamics of the system can be obtained as a set of partial differential equations based upon the Lagrangian function. The differential equations are derived from the principle that the system evolves such as to make the action of the system, ∫Ldt, an extreme.

The calculus of variation provides the conditions on the variation in the state variables over time that results in an extremum of the action ∫Ldt. These conditions are known as the Euler-Lagrange equations.

For example, consider a point particle of mass m in a uniform gravitational field in which the potential energy is given by V=mgz, where z is the height above an arbitrary point and g is a parameter representing the the strength of the gravitational field. The variable z is the only state variable of the system. The Lagrangian L of the system is

#### L = ½m(dz/dt)² − mgz

Let (dz/dt) be denoted as v. The Euler-Lagrange equation for the system is

This reduces to

#### d(mv)/dt −(− mg) = 0 which further reduces to dv/dt = −g or, equivalently d²z/dt² = −g

Thus the particle moves downward at an accelerating rate that is independent of the mass of the particle.

## The Lagrangian of a System Having an Equilibrium Point

Let Q be the vector of the state variables of the system, its generalized coordinates and U be the vector of the time rates of change of those variables. An equilibrium point of the system is a value of the state variable, say Q0, such that the corresponding U vector is the zero vector.

The system can be rewritten in terms of state variables which are deviations from the equilibrium point. For vanishingly small deviations the system is linear. The linear system will have a set of oscillations of specific frequencies. These are called the normal modes of the system and its spectrum.

## The Lagrangian of a Field

Let L be the Lagrangian density function at a point in space (x, y, z). Then the Lagrangian for the system is

#### L = ∫Ldxdydz and its action is ∫Ldxdydzdt

There are corresponding Euler-Lagrange equations which must be fulfilled for the system to achieve an extreme of the action, a minimum, a maximum or a point of inflection.

## The Lagrangian of an Electromagnetic Field

An electric field can be described by the force on a unit charge at every point in space. This force per unit charge is a 3 dimensional vector. Let the electric field vector be denoted by E. The component of the electric field along the i axis is denoted as Ei, where i can be 1, 2 or 3. Likewise the magnetic field is denoted as B and its components as Bi. The electromagnetic field can also be specified in terms of a scalar potential function V and a vector potential function A. The relationship between these two representations of an electromagnetic field is

#### E = −∇V − ∂A/∂t B = ∇ × A

where V is the gradient of the scalar field V and ×A is the curl of the vector field A.

A 4 dimensional vector potential A, in which the index runs from 0 to 3, can be defined in which the first (zeroeth) component is the potential function V and the other three are those of A; i.e.,

#### A = (V, A) and thus A0 = V

Therefore −V − ∂A/∂t can be represented as something in the nature of a 4 dimensional gradient of A. There is a special notation for this operation which will be covered later.

There are two other variables that are relevant for representing an electromagnetic field, a 3 dimensional current vector J and a scalar charge density ρ. These can be used to create a 4 dimensional vector J=(ρ, J).

The Lagrangian density function for the electromagnetic field is then

#### L = ½(E·E − B·B) − ρV + J·A

The Euler-Lagrange equations for the above Lagrangian density function turn out to be the Maxwell equations for an electromagnetic field.

## Tensorial Notation

The generalization and hence more general term for vectors and matrices is tensor. In the notation for tensors there is an important difference between variables with subscripts and variables with superscripts. This also applies to symbols for derivatives.

The symbols for space variable are x1, x2 and x3. Time is denoted as the zeroeth variable x0. (Some mathematical physicists denote time as the fourth variable.) Greek letters are used to denote indices that go from 0 to 3, whereas an index that ranges from 1 to 3 is denoted by a Latin letter.

The magnitude of any vector a=(a0, a1, a2, a3) is given by

#### |a| = ΣμΣνgμνaμaν

where the matrix gμν is known as the metric tensor.

The equations are much simplified if a repeated index in a single term is always summed. This is the Einstein convention. Thus

#### |a| = gμνaμaν

For physical theory about the world the metric tensor is taken to be a diagonal matrix with (+l, −1, −1, −1) on the diagonal.

For the above metric tensor the relationship between a variable with superscripts and one with subscripts is that

#### aμ = (a0, a1, a2, a3) = ( a0, −a1, −a2, −a3)

The notation for derivatives is especially opaque.

#### ∂μ = (∂/∂x0, ∂/∂x1, ∂/∂x2, ∂/∂x3) which can be represented as ∂μ = (∂0, ∇)

On the other hand,

This means that

The expression

#### ∂²/∂t² − ∇² can be represented as ∂μ∂μor, equivalently as ∂μ∂μ

When an index is a Latin letter it means that it goes form 1 to 3. Forexample,

#### −∇V − ∂ A/∂t = ∂iA0 −∂0Ai

This is the expression that was mentioned previously as being in the nature of a 4 dimensional version of .

## Lagrangian Analysis of a Scalar Field

Let φ be a scalar field, a quantity defined at all points of space. Consider a system in which its Lagrangian density function depends only on φ and the gradient of φ

#### L = L(φ, ∂μφ)

For example, φ might be pressure in a container. Then ∂μφ would give the flow directions.

The action for the system is

#### S = ∫L(φ, ∂μφ)dx4

where dx4=dtdxdydz.

Now consider a variation on the state variables such that

#### x → x+δx and thus φ(x) → φ(x)+δφ(x)

This means that the variation in the Lagrangian density is

#### δL = (∂L/∂φ)δφ + (∂L/∂(∂μφ))δ(∂μφ)

The variation in the action is then

#### δS = ∫[(∂L/∂φ)δφ + (∂L/∂(∂μφ))δ(∂μφ)]d4x

The term δ(∂μ) reduces to ∂μ(δφ). Now consider the second term in the integral

#### ∫[(∂L/∂(∂μφ))(∂μδφ)]d4x

According to Gordon Kane an integration by parts operation will put this integral into the form

#### −∫[∂μ(∂μφ))(∂μδφ)δ]d4x

That is to say, the above integral can be represented as ∫UdV, which is equal to {UV − ∫VdU}. When UV is evaluated over the boundaries of the region of integration it is zero, again according to Gordon Kane.

The above evaluation of the integral means that

#### δS = ∫[(∂L/∂φ) − ∂μ(∂L/∂(∂μ))δφ]d4x

Since δφ is arbitrary, in order for δS to be zero it is necessary that

#### (∂L/∂φ) − ∂μ(∂L/∂(∂μ)) = 0

This is the Euler-Lagrange equation for the scalar field.

## Application for a Particular Scalar Field

Let the Lagrangian for a scalar field φ(x) be

#### L = ½[∂μφ∂μφ − m²φ²]

where the parameter m is mass.

The first term is the kinetic energy K and the second term is the negative of the potential energy V; i.e., L = K − V.

The derivative ∂L/∂φ is −m²φ. The derivative ∂L/∂(∂μ) is ½∂μ. Therefore the Euler-Lagrange equation evaluates to

#### −m²φ + ½∂μ∂μφ = 0

The second term is equivalent to ½[∂0²φ − ∇²φ].

In more conventional notation this is

#### ½[∂²φ/∂t² − ∇²φ].

Therefore the Euler-Lagrange equation for the field is

#### ∂²φ/∂t² = ∇²φ + 2m²φ

If m is equal to zero this is the wave equation

#### ∂²φ/∂t² = ∇²φ

If m is not equal to zero it is a form of the Klein-Gordon equation in natural units; i.e., with the speed of light and Planck's constant divided by 2p set equal to unity.

## An Application to an Electromagnetic Field

Let Ei and Bi for i=1,2,3 be the components of the electrical and magnetic field intensities, respectively. Let Ai for i=1, 2, 3 be the components of the vector potential for the field.

A two-index antisymmmetric tensor F may be defined for the electromagnetic field as follows.

#### F0i = −Ai = ∂0Ai − ∂iA0 Fij =∂iAj − ∂jAi = εijkBk

The tensor εijk is such that εijk=1 if ijk is an even permuation of 123, is −1 for an odd permutaion and equals zero for any other repeated index.

The tensor F allows the Lagrangian for the electromagnetic field to be written as

#### L = −¼FμνFμν − JμAμ

Now the analysis will go back to the Lagrangian of the electromagnetic field as

#### L = ½(E·E − B·B) − ρV + J·A

Some notable properties of this Lagrangian are:

#### ∂L/∂V = −ρ ∂L/∂(∂V/∂xi) = −Ei

(To be continued.)

## The Lagrangian Density Functions of Particle Physics

In addition to the case of a real scalar function shown above, the following are utilized in particle physics.

### A Complex Scalar Field

For this case the complex field function φ satisfies the condition (∂μμ + m²)φ = 0 and the Langrangian density function is

#### L = (∂μφ)*(∂μφ) − m²φ*φ

where the asterisk * denotes the complex conjugate.

### A Fermion Field

Let ψ(x) be the two component spinor wave function for a spin-½ fermion and let m be its mass. Then its Lagrangian density function is

#### L = ψ(iγμ∂μ − m)ψ

where i is the imaginary unit √−1. The γ's are related to the Pauli spin matrices and ψ is the product of γ0 and the complex conjugate of ψ. The wave function ψ satisfies the Dirac equation

## Langrangian Dynamics Applied to Particle Physics

Consider a system with the Lagrangian

#### L = K − V(φ)

where φ is the field intensity.

The kinetic energy intensity K is given by

#### K = ½∂νφ∂νφ

with summation over ν.

The potential enegy function is of the form

#### V(φ) = (½μ2φ2 + ¼λφ4)

where μ and λ are parameters of the potential function.

The term λφ4 represents an interaction which is said to be of strenth λ. The parameter λ is presumed to be positive.

The potential energy function V has the symmetry

#### V(−φ) = V(φ)

The other way of describing this property is that the potential energy function is invariant under the transformation φ → −φ.

The mass for the system (particle) is determined by the behavior of the potential function near to its minimum value. The minimum value of the potential energy function is also known as the ground state and more obscurely as the vacuum.

If μ is a real number and hence μ² is a positive real number then the potential energy function has the shape shown below and the minimum V is V(0).

For this case the mass of the particle is zero.

On the other hand if μ² is negative then the potential energy function has the following, more interesting shape.

In order for μ² to be negative μ must be an imaginary number. The minimum value of V is obviously not V(0). This case gives rise to a positive mass for the particle represented by the Lagrangian. When the Lagrangian has symmetry but the minimum value of V is not zero the situation is called broken symmetry.

## Broken Symmetry

(To be continued.)

## Comment

It is amazing that anyone would believe that such relatively simple manipulations of Lagrangians could tell us anything about the real world. It is immeasurably more amazing that in fact such analysis does tell us profound things about the real world. However, there is the precedent of the theorems of Emma Noether in which in the most famous one she found that if the Lagrangian of a physical system is invariant under continuous transformations with respect to time and location then energy and momentum are conserved. In the case of the Noether theorems the conservation laws were known, or at least strongly suspected to hold. In the case of the Lagrangian analysis for particle physics previously unknown relationships are being revealed.

Sources:

• Gordon Kane, Modern Elementary Particle Physics, Addison-Wesley Publishing Co., Menlo Park, California, 1993.
• T.D. Lee. Particle Physics and Introduction to Field Theory, Harwood Academic Publishers, New York, 1981.
• W.M. Gibson and B.R. Pollard, Symmetry Principles in Elementary Particle Physics, Cambridge University Press, Cambridge, 1980.

For material on Yang-Mills fields see Yang-Mills.

For material on Special Unitary Groups and Algebras see SU(2) and SU(3).