Physics+ Nonconservative Lagrangian: UNIZOR.COM - Physics+ 4 All - Lagrangian
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This lecture introduces the concept of applying Lagrangian mechanics to non-conservative systems, specifically addressing scenarios where forces depend on velocity rather than just position. The presenter uses a classic example of a stone falling through water to illustrate this challenge; in addition to gravity acting as a potential force, there is a resistive drag force proportional to the object's speed. While Newtonian mechanics handles such simple one-dimensional problems straightforwardly by balancing mass times acceleration against these opposing forces, Lagrangian formalism offers a different perspective that becomes increasingly valuable for complex systems with multiple degrees of freedom or constraints. The goal here is not merely to solve this specific differential equation but to demonstrate how the standard Euler-Lagrange equations can be adapted when energy conservation does not hold due to dissipative effects like fluid resistance.
To construct an equivalent Lagrangian function $L$ that yields the same physical predictions as Newton's second law, the presenter employs a clever mathematical technique involving integrating factors and algebraic manipulation of the equation of motion. By multiplying the rearranged Newtonian equation by an exponential term dependent on time ($e^{kt/m}$), the expression can be rewritten so that both sides appear as partial derivatives with respect to position $x$ and velocity $\dot{x}$. This allows for the definition of a new Lagrangian function, which initially looks like the standard kinetic energy minus potential energy but is scaled by this specific time-dependent multiplier. The resulting form effectively mimics the conservative structure ($T - U$) while explicitly incorporating the non-conservative nature of the system through the exponential factor that varies with time.
The final derived Lagrangian highlights a crucial distinction between conservative and non-conservative systems: in standard mechanics, energy is conserved because the potential depends only on position, but here the explicit dependence on time means total mechanical energy is not constant. As the stone falls, it accelerates until drag balances gravity, reaching a terminal velocity where acceleration drops to zero; this physical behavior corresponds mathematically to the solution of the modified Euler-Lagrange equation derived from the new function. Although Lagrangian mechanics loses some of its elegant features like strict energy conservation in non-conservative cases and can become difficult for highly complex dissipative systems, it remains a powerful tool that successfully bridges Newtonian dynamics with variational principles even when friction or air resistance is involved.
Read the full video transcript
Hi, I'm Zor. Welcome to Inor Education.
I have decided to put a little bit more
information into the grand chapter um
especially for uh non-conservative
systems. Before we were talking about
only conservative systems like for
example um some kind of a object is
moving in the gravitational field. Well,
gravitational field is potential field.
It has a function which is called
potential and the force depends on the
position. But in some cases the force
depends not only on position but also
for example on speed that complicates
the picture and in the form which we
were using it before cannot actually be
used. So today is this particular
example of non-conservative system and
how to build lrrenjan for this system.
Okay. So this lecture is part of the
course
um physics plus it's a chapter called
lranjan and the lecture is called
non-conservative
lanjan.
Um now this course has prerequisites.
Um
before physics plus I had physics for
teens and also I have math courses math
for teens and math plus. So I presume
that all these uh prerequisites are
totally familiar with you because I will
use some concepts which I was basically
using introducing before. So this is
just a continuation. Now the website
unisur.com is totally free. There are no
advertisement.
Um you don't have to sign in, no
subscription, totally free thing, pure
knowledge for your consumption. Um every
lecture has written part like notes
and they are written usually in a style
of textbook. So you can um watch the
lecture uh video, you can read the
corresponding text which is on the same
web page on unisord.com
and that would help you to understand
material much better obviously. So you
have a textbook and you have a video
presentation of the same material
basically on the same web page.
Um now there are some exams not not in
this particular course but in previous
courses there are exams which I um which
you can take as many times as you want
just to selfch check yourself. Um there
are some provisions for supervised
education uh on the website again
totally free. All right so let's get
back to business.
Um now as I was saying our uh lr John we
were familiar with which typically was
like l is equal to t minus u uh lran
john um kinetic energy and u
potential energy. Now kinetic energy was
more or less like
12 m²
or maybe some other quadratic form. Um
the potential energy was just a function
of position.
So if that is true then well the gjan of
this type more or less fits. But now
let's consider a completely different
problem.
Let's say you have a surface of water
and you drop a stone.
Now the stone goes down the water. Why?
Well, there are two different forces.
The first force is obviously
its weight.
Now let's say we have x
um axis uh directed downwards. So there
is a force which is its weight and
another force is the force of resistance
of water. Now the water is such a um
media that um the resistance actually is
not constant. It depends on the speed.
it's actually proportional to speed more
or less within certain um kind of
precision things. So I assume that the
force which is actually
u directed against the motion is
proportional
to
uh to its speed.
Okay. So there are two forces and first
let's do what u classical Newtonian
mechanics is doing. In this case we have
two forces in this case they're uh
one-dimensional. So
introducing lranjan will not actually do
a lot of new things and uh will not be
very useful. Granjan is good in the
complex systems. This is a simple one
but it's just an example just to show
how lenjan would be working in
non-conservative case. So simple case we
have two forces along the same line x
axis this is uh the positive direction
this is negative direction. So the um
um
uh the Newton's equation
the Newton's equation would be what?
That the force is equal to acceleration
right
mass time acceleration.
So mass time
second derivative of time
x is coordinate. So this is m and this
is acceleration a. Now this is force
basically uh mass times acceleration.
And what is the force? The force is mg
minus
k first derivative.
Speed is first derivative of position.
So this is my second Newton's law.
And uh
it's actually rather simple differential
equation and I'm going to basically not
not to solve it. I'll just give you the
result because solution is completely
outside of the scope of this lecture. It
goes to differential equation and it's
easy. So for those people who are
familiar with differential equation,
they can actually try to solve it. And
the first step would be uh instead of u
first derivative you can put just
another function y
which is the first derivative. So now
you have the derivative only to the
first degree right. So my is equal to mg
minus k y. So this is differential
equation of the first order uh
relatively uh easy to solve and I'm not
going to do it and I'm going to write
immediately the result of this just for
you to know that this differential
equation has an interesting result and
what is the result
of t is equal to
mg
this is G
gravitational constant
divided by K T minus
M²
G / K²
if K
T / MUS
well it's rather complex formula but
look
>> [clears throat]
>> It satisfies u basically this equation
and it satisfies
x sub0 is equal to zero and uh speed
at the time is equal to zero. My
position is on the surface and there is
no speed. So I just put it there and let
it go.
So this is the equation which basically
corresponds to
this particular
uh condition.
Oh I think it's plus here
not minus.
Yeah. So it's plus.
Now if t is equal to zero this is equal
to zero and this is zero. So it's zero.
And then I can put the expressions for
the first and the second derivative.
MG
divided by K 1 - E
minus KT / M.
And the second derivative acceleration
is equal to G * E minus KT / M. Okay. So
I'm just giving it to you as pure math
thing. I'm not going to spend any time
on uh actually solving this or taking
the derivative. It's all basically kind
of elementary stuff. I'm not going to uh
spend any time on it. But what we
actually can do from it, we do some kind
of a logical conclusion. Look,
acceleration is always positive.
Although with t going to infinity
this thing goes to zero. So my
acceleration while positive still going
to zero
like reverse exponential thing my
acceleration graph of acceleration would
be like this.
This is one
at t is equal to zero.
Okay. Now, which means if acceleration
is positive, although it just goes to
zero, but it's positive, which means
speed is increasing.
Positive acceleration. So, speed is
increasing. So, this is an increasing
function. However, since acceleration
goes to zero, my increase of the speed
is also
going down. And uh the whole thing
actually as t goes to infinity so this
is zero it goes to maximums basically
it's a maximum speed the limit speed
limit is mg divided by k this is 1 minus
so this is zero so it will be only mg
divided by k so this is a limit speed
eventually as the stone goes down in the
water it goes faster and faster and
faster however Ever it's not an infinite
increase of the speed. The speed will
increase up to this limit not reaching
this limit. So it will be faster and
faster but still and eventually it will
be from from the observe uh from the
observer
after certain amount of time when this
thing is really substantially zero it
will look like the speed is constant. So
it will constant with a constant speed
going down uh in water. So this is my
basically research based on equation and
its solution
and uh an analysis of the speed and
acceleration.
Fine. This is Newtonian thing. It's not
very difficult at all. So there is no
need like inventing John etc. But I'm
using this as an example of um using
lranjian mechanics to get some formula
for lranjan and oiler lrange equation in
this particular case which will be
definitely different from conservative
system.
Why? Because because of this force which
is which depends on u on the speed. All
right. So let's go to the current job.
So this is my Newtonian
second law.
Now if lranjan
exists for this system then the oiler
lrange equation which is this
now first we go by time right
of partial derivative
x x prime t by d x prime
= to d l
x prime d
x. So this is my oiler lrange equation.
So if Ljan to this system exists
then solution of this equation and this
equation I mean L is some kind of a
formula which depends on X X prime and T
then solution would be X of T some kind
of a function should be the same as
solution to this thing. So these two
equations must be equivalent.
Now how can I come up with this
particular function L expression which
depends on X X prime and T. How can I
come up with this in such a way that
this equation is equivalent to this
equation? Well from the first glance it
doesn't seem to be easy. But um some
smart people actually um came up with a
very interesting approach to this
problem. Let's take this equation and
try to modify it in such a way that it
will look like this equation where else
some kind of a function. So that's what
I'm going to do. I'm following um those
smart people who have already done it
for me. So first of all we will um
modify this equation. We will divide it
by m
that would be easy.
And instead of K I will put
K / M
and I will even do it better. I will put
this to the left. So it will be plus
and G would be to the right.
So it will be plus this equals G.
So this is the same Newtonian second
law. I'm just rearranging a little bit.
So I will use this as my starting point
and I will try to change it in such a
way that it will look like this one.
Okay. So what actually was uh kind of a
ingenious
um
guess was let's multiply both sides of
this equation by e to the kt / m.
So what I will have is this. I will have
this
um I will not use uh t it's assumed
basically plus this
equals this
right
just multiply by this multiplier
which is never equals to zero by the
way. So I did not really introduce
anything new. It's equivalent
um it's equivalent equation equivalent
to this one. Whatever is solution to
this is solution to this and vice vice
versa. Now look at this expression.
I'm just saying that I can recognize
this as the derivative by time of this
function. Why? That's the um product of
two functions of t. This is a function
of t. This is a function of t. So it's
this one times derivative of this which
is this
plus
this
time derivative of this which is e to
the power of kt / m times the
exponential coefficient at expon at at
exponent it would be k / m. So this is
the left part. Okay.
Okay, [clears throat]
I need this to be equal to this, right?
Well, that's easy
because this is function of t and this
is partial derivative only by x prime by
the speed, right? So, I can actually
have dt
d by dx prime of what?
Now this is function of t I can put it
as is
and for having
okay
so partial derivative by x1 x prime now
this is not related to x prime so it's
like a multiplier where partial
derivative so it's only depends on x
prime and partial and derivative of 12
of x prime squared is obviously two uh
cancel with two and x prime. So this is
what it is. So this is my left part and
it looks very much like this.
Now what's on the right part? Well, on
the right part I have to have a partial
derivative by x. But this is doesn't
depend on x. So basically if I will I I
will have it as a partial derivative by
x of e ^
um kt / m g * x
partial derivative of x would be this
right
now I can say that these are equal
this is equal right so I'm just
converting converting this thing into
slightly different format but now it
looks much better much closer the only
problem is this is the same function L
and L here I have two different
functions however what's very important
this is partial derivative by X prime
and this thing has no x prime so I can
always add this to this
without changing
anything.
So if instead of this I will put this
plus this derivative by x prime will not
change because this thing is not
dependent on x prime. So I can always
say that this is d by dt
d by dx prime
e to the power kt
/ m
x prime²
um
uh
plus
e to the kt t / m
gx
that's on the left side.
Now on the right side I have partial
derivative by x. This thing doesn't
really depend on x. So I can add this to
this
and that would be d by dx of again of
the same
thing
which means this same thing
this one e to the power kt / m is the
same on both sides. So I can have this
as 12 x prime squar plus
mgx.
It can be my l of t of x
x prime and t.
So with this L
this particular oiler lrange equation is
exactly equivalent to this one because I
was just converting with uh with
absolutely equivalent
transformations.
Uh no no this is not m this is just gx
I'm sorry m is out.
All right. So this is my function but I
would like actually to be a little bit
more physical so to speak. Now if this
is function if I will multiply by
constant both sides it will be the same
thing. So instead of this I will put
this
12 m and m here.
This is my lanian. Why did they do this?
Because this looks like a t.
This looks like minus u minus because x
is going down. So as x is increasing,
potential energy is decreasing. Right?
So what is my final formula? used to be
remember L is equal to T minus U for
conservative system and for this
particular system it's E to the power KT
/ M * T minus U looks like it but there
is one multiplier which depends on on on
time.
So that's what's very important. So we
have come up with
a lanjan which is kind of resembling in
some way the non-conservative system but
be uh the conservative system but
because this is a non-conservative and
time dependent this time dependency this
particular case this particular problem
is reflected in this multiplier which is
explicitly depends on on time and since
it's explicitly depends on time there is
no such thing as um conserv conservation
of energy and there are some nice you
see many very nice features of lrrenjan
and lrrenjan mechanics are actually for
conservative systems non-conservative
systems present problems now in this
particular case we have come up with
certain solution which results in a very
interesting kind of a function which I I
I I like that it resembles the
conservative system with just one
multiplier In the more sophisticated
cases, it's probably much more complex.
We are not going to go. However, this is
an example of using plunjan mechanics
for a non-conservative system. So, it is
possible although it loses its um
many of its nice features like uh
conservation laws and and and some
others. So lanjan mechanic is nice for
conservative systems and in many cases
it gives you a lot of advantages like
for instance generalized coordinates.
This is not generalized coordinates and
again in some more sophisticated case uh
it will not be possible to do like a
relatively simple conversion from a
Newtonian torren
mechanics. So that's that's what it is.
I just wanted to give you this
particular example. I do suggest you
reading the uh the notes for this
lecture. Uh they are a little bit more
detailed but not by much. But still
what's very important is approach
approach is take the Newtonian second
law and convert it into format which is
looks like lranjan. That's what actually
was done kind of artificial. Uh I agree
but well whatever I mean it works.
All right. So thanks very much and uh
good luck.