What is the Lagrangian and how is it used in physics?

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SUMMARY

The Lagrangian is a fundamental concept in physics, defined as the difference between kinetic energy and potential energy (L = T - V). It is utilized in the formulation of classical mechanics through the principle of least action, which states that the path taken by a particle is the one that minimizes the action integral. The discussion emphasizes the importance of understanding the Lagrangian before advancing to more complex theories such as quantum mechanics and general relativity. Recommended resources include Leonard Susskind's Classical Mechanics Lectures and Landau's physics texts for deeper insights into the Lagrangian formalism.

PREREQUISITES
  • Understanding of Newtonian mechanics
  • Familiarity with calculus, particularly integrals and derivatives
  • Basic knowledge of energy concepts (kinetic and potential energy)
  • Introduction to functional analysis and variational calculus
NEXT STEPS
  • Study Leonard Susskind's Classical Mechanics Lectures for a comprehensive understanding of the Lagrangian.
  • Read Landau's first book in his series on physics to explore the derivation of the Lagrangian through symmetry principles.
  • Learn about the Euler-Lagrange equation and its applications in deriving equations of motion.
  • Investigate the principle of least action and its implications in modern physics, including quantum field theory.
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Students and professionals in physics, particularly those interested in classical mechanics, quantum mechanics, and theoretical physics. This discussion is beneficial for anyone seeking to understand the foundational principles that govern motion and energy in physical systems.

Justice Hunter
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So i actually have many words that i know of, and are familiar with such as :

The Hamiltonian Operator
The Hermitian Operator
The Lagrangian
Eigen Values/States

However, i am struggling with how these things work, and when to apply them, and what they actually mean. Many of the physics lectures i watch tend to glaze over them.

For simplicity sake, let's just start with the Lagrangian. What exactly is it? When is it applied, and can someone offer an example of its use?
 
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I will recommend you very highly stanford Leonard Susskind Lectures.I watched Classical Mechanics Lectures 2008 I guess.Perfect explanation of Lagrange.If you know calculus definitely watch it.
 
RyanH42 said:
I will recommend you very highly stanford Leonard Susskind Lectures.I watched Classical Mechanics Lectures 2008 I guess.Perfect explanation of Lagrange.If you know calculus definitely watch it.

Ahh you its funny you say that, that's where i picked up most of those terms, from Susskind's lectures online. Sometimes he just throws around those words and i don't have a clue what they mean.

I totally skipped his classical mechanics lectures though, i went straight to GR and QM lol! So i'll definitely take your advice to heart and watch those.
 
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The "Hamiltonian" is the total energy operator. The "Lagrangian" is the operator that gives the difference between potential energy and kinetic energy (rather than the sum like the "Hamiltonian").
There is no operator called "the Hermitian" operator. Any operator is an "Hermitian" operator if it is its own conjugate transpose. In particular, its eigenvalues are always real numbers.

An "eigenvalue" for an operator, A, is a number, \lambda such that there exist non-zero vectors, v, such that Av= \lambda v. Those vectors are called "eigenvectors". Eigenvectors have the nice property that the operator, restricted to an eigenvector or multiple of an eigenvector is just "multiplying by a number" so very simple. If you can find a basis for your vector space, consisting entirely of eigenvectors, (i.e. an Hermitian operator) the operator can be written in a very simple form.

You can't just "jump" to quantum theory and relativity, ignoring all of the preliminary physics (and mathematics)!
 
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A Lagrangian is a function that is used when you take Newtonian mechanics using vector methods and such, and reformulate it in an analytic method. To define what it means and such is basically a few lectures worth of material on advanced classical mechanics. In general, it is the Kinetic energy of a system minus its potential energy. When you integrate this function over time you get a scalar called the action. From this point on it gets pretty technical. It's taken as a postulate that varying the action to first order should be 0 for the trajectory of motion. You should read Landau's first book in his series on physics, he derives very beautifully why the lagrangian is what it is by symmetry principles. The hamiltonian is again a reformulation. This time you go from the langrian to the hamiltonian via a legendre transform. the lagrangian does not always have to "look" like the mechanical kinetic energy-potential and the hamiltonian does not always look like the regular mechanical energy of a system.

You really should get a firm grasp on the subject before moving on. All modern theories are formulated in terms of Action and lagrangian formalisms. This inlcludes quantum field theory and string theory. General Relativity also has an action formulation.
 
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Justice Hunter said:
For simplicity sake, let's just start with the Lagrangian. What exactly is it? When is it applied, and can someone offer an example of its use?

The Lagrangian is an object called a functional, a device that returns a number for any given function. For instance, a definite integral is a simple case of functional. We also have the functional derivative, which explains how the value of the functional will change when the function put into it is changed, defined:

(δF[f(x)]/δf(x)) = limε→0 (1/ε)(F[f(y) + εδ(x - y)] - F[f(y)]) Where F is some functional, f(x) some function, y is a dummy variable, and δ(x-y) is a Dirac delta function. The subject of calculus of variations deals with operations on functionals.

When you're considering the trajectory of a particle, there are two functionals you want to think of: the averages over some duration τ of potential energy V and kinetic energy T of a particle following a trajectory x(t) connecting two points a and b. These are defined:

Tave = τ-10τ(1/2)m[xt(t)]2dt

Vave = τ-10τV[x(t)]dt

We can take the functional derivatives of Vave and Tave to find that

δVave[x(t)]/δx(t) = δTave[x(t)]/δx(t)

meaning that if we vary the trajectory x(t) by a small amount, the average kinetic energy and average potential energy for the duration will each change by the same amount, or that the difference between the average kinetic energy and average potential energy does not change as the trajectory changes

(δ/δx(t))(Tave[x(t)] - Vave[x(t)]) = 0

That observation motivates us to define the Lagrangian, L = T-V. The Lagrangian is special because it does not change as the particle moves through its trajectory. We can also define a quantity S called the action, which is the time integral from 0 to τ of the Lagrangian, measured in Joule-Seconds (if you've taken an elementary QM course, reflect on the fact that Planck's constant h is also defined in Joule-Seconds). We also have Hamilton's Principle of Least Action,

δS/δx(t) = 0

which tells us that the path that will be taken by a particle between points a and b is the one for which the action will be stationary (a maximum, minimum, or saddle trajectory, analogous to maxima and minima in calculus). By using the Lagrangian and the Principle of Least Action, we can we can derive the Euler-Lagrange equation, and then from there we can solve the Euler-Lagrange equation to determine the laws of motion for the system. Intuitively, the Lagrangian and the action contain the dynamics for a system.

Here's an example: https://en.wikipedia.org/wiki/Lagrangian#An_example_from_classical_mechanics
 
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jack476 said:
The Lagrangian is an object called a functional, a device that returns a number for any given function. For instance, a definite integral is a simple case of functional. We also have the functional derivative, which explains how the value of the functional will change when the function put into it is changed, defined:

Thanks so much for the detailed response! I think i understand now, Thank You!
 
Here's is a simple derivation of an action principle. It is fairly easy to prove that the solution of Newton's equations for particle motion,

##m {d^2 x \over dt^2} = F##

minimizes the action:

##S = \int_{t_1}^{t_2} \big[ {1 \over 2} m \dot{x}^2 - V (x) \big] dt##

where the integrand ##\mathcal{L} = {1 \over 2} m \dot{x}^2 - V (x)## is called the Lagrangian.

Denote by ##x_c (t)## the motion which minimizes the action. We consider an alternative `motion' given by ##x (t) = x_c (t) + \alpha \eta (t)## where ##\alpha## is a parameter we are free to vary and ##\eta (t)## is an arbitrary function (called a `test' function). The only condition we impose is that the initial and final positions are fixed, in other words ##\eta (t_1) = \eta (t_2) = 0##.

We can calculate the action of this alternative motion ##x (t) = x_c (t) + \alpha \eta (t)## - making it a function of ##\alpha##:

##S(\alpha) = \int_{t_1}^{t_2} \big[ {1 \over 2} m (\dot{x}_c + \alpha \dot{\eta})^2 - V (x_c + \alpha \eta) \big] dt##.

As ##x_c (t)## minimizes the action, ##S(\alpha)## will have a minimum at ##\alpha = 0## for any test function ##\eta (t)##. This can be expressed:

##{\partial S (\alpha = 0) \over \partial \alpha} = 0##.

Let us expand ##S(\alpha)## in powers of ##\alpha##:

##S(\alpha) = \int_{t_1}^{t_2} \big[ {1 \over 2} m (\dot{x}_c + \alpha \dot{\eta})^2 - V (x_c + \alpha \eta) \big] dt =##
##= \int_{t_1}^{t_2} \big[ {1 \over 2} m \dot{x}_c^2 - V(x_c) + \alpha m \dot{x}_c \dot{\eta} - \alpha {\partial V \over \partial x} \eta + \mathcal{O} (\alpha^2) \big] dt##

(where ## \mathcal{O} (\alpha^2)## denotes terms of order ##\alpha^2## and greater). The requirement ##\partial S (\alpha = 0) / \partial \alpha = 0## gives:

##\int_{t_1}^{t_2} \big[ m \dot{x}_c \dot{\eta} (t) - {\partial V \over \partial x} \eta (t) \big] dt = 0##

upon integrating by parts, we obtain:

##[m \dot{x}_c \eta (t)]_{t_1}^{t_2} - \int_{t_1}^{t_2} \big[ m \ddot{x}_c + {\partial V \over \partial x} \big] \eta (t) dt = 0##

Using ##\eta (t_1) = \eta (t_2) = 0##, this is reduces to:

##\int_{t_1}^{t_2} \big[ m \ddot{x}_c + {\partial V (x_c) \over \partial x} \big] \eta (t) dt = 0##.

This is true for all test functions ##\eta (t)##, we can imagine test functions `concentrated' at each particular time between ##t_1## and ##t_2## and conclude that what is in the square brackets vanishes, giving:

##m {d^2 x_c \over dt^2} = - {\partial V (x_c) \over \partial x} = F##,

the required result.
 
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