For more information, please see full course syllabus of Differential Equations
For more information, please see full course syllabus of Differential Equations
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Euler Equations
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- Intro 0:00
- Lesson Overview 0:11
- Euler Equation
- Real, Distinct Roots
- Real, Repeated Roots
- Complex Roots
- Example 1 3:51
- Example 2 6:20
- Example 3 8:27
- Example 4 13:04
- Example 5 15:31
- Example 6 18:31
Differential Equations Online Course
Transcription: Euler Equations
Hi welcome back to the differential equations lectures here on www.educator.com, my name is Will Murray and today we are going study Euler equations, let us jump right in.0000
Euler equations have a very special form, they are the form x2 y″ + a constant which I’m calling α × XY′ + β (another constant) × y=0.0012
The idea there is that there is this pattern of descending powers on the x, this is very important.0027
We got an x2 here, we got an x here, and you want to think this is x 1, you want to think that this is x0 because it is just a constant.0036
You really have to have that exact pattern of the powers, x2, x and x0 in order to make the order of the equations work.0045
If you do have that pattern then there is a very easy solution it is basically xr.0054
Let me show you how to figure out what r is, what you are going to do is you are going to solve the characteristic equation for r and there is a little subtlety here.0060
Basically you take the coefficients from the order equation but there is a small change which is just instead taking α and β, you take α – 1 and β.0071
You solve this characteristic equation r2 + α – 1r + β=0.0083
That is just a quadratic polynomial, you can solve that by factoring, by quadratic formula, and whatever works for you to solve that and you will get 2 roots for r, you get an r1 and r2.0090
This is not really hard, this is just algebra, you could get 2 real roots, so you could get r1=3, r2=5 or something like that.0106
You could get 1 repeated root, meaning you will get a double root or you could get 2 roots that are complex conjugates.0118
Something like a + π and a – π, that is if you are on a quadratic formula and you get a negative number under the square root sign, then you are going to get 2 complex conjugate roots.0125
Let me tell you what to do in each one of those situations and how you will write down the solution to the differential equation.0136
If you have real distinct roots, meaning 2 different real roots the general solution to the equation is just xr1 × constant and xr2 × another constant.0144
It is very easy there if you have repeated roots, same copy of root appears you have xr1 and xr1 × natural log of x.0155
Again, multiplying each one by a constant and if you have complex roots then it will always occur in conjugate pairs.0166
Remember that the quadratic formula is something (+ or -) the square root of something.0173
If you get a negative number under a square root then you will end up getting a conjugate pair, something like a (+ or -) π.0182
It is a little more complicated if you do that but it is just a formula to remember.0191
It is xa × cos(x) of logx to the b and xa × sin of natural log of xb.0195
Those are your 2 fundamental solutions and you just multiply each one by an arbitrary constant and you will get your general solution.0208
That is pretty much all you need to know for Euler equations, you solve the characteristic equation, get the 2 roots.0215
Just depending on which of these 3 situations it is, you just drop it in to one of these 3 formulas, let us try that out with some examples.0223
In our first example, I want to find the general solution to x2 y″ – 3xy′ + 3y=0.0231
We got this Euler pattern on the coefficient x2, x and then a constant here, so it is an Euler equation.0240
The α here is -3 because that is the coefficient here, the β is 3 and remember the characteristic equation is always r2 + α- 1r + β=0.0249
That is the equation that you always solve for r and in this case we have r2,0272
Now α is -3, so α – 1 is -4, this is actually -4r and β is 3, +3 =0.0280
That equation factors quite nicely that is r-1 × r-3=0.0292
Our 2 values of r are 1 and 3, r=1 and r=3, now we can drop those right into the general solution.0303
The general solution is c1 × x + c2 x3, that is the solution to the differential equation.0317
It is a really nice relief that this Euler’s equations are much easier than some of the other things that we have been doing recently like series solution.0336
Let me recap quickly how we worked that out, we noticed that this was an Euler equation because it has that descending pattern of powers x2, x, and constant.0345
We read off our values of α and β, just the coefficients there -3 and 3.0356
Drop them into this characteristic equation, the key point there is to remember to subtract 1 from the alphas.0362
We got r2 -4 +3 =0, factor it out, get our roots and those become the powers and we get our general solution.0367
Let us go ahead and try another one, we still have an Euler equation here because the powers on x is descending.0380
We have x2, x, and a constant, our α here is -7, β is 16.0389
We are going to use our generic characteristic equation r2 + α -1r + β=0.0402
Our α is -7 so α – 1 is -8, -8r + 16 = 0.0412
(r) factors into r-42=0, we get the double root at r =4 or 4.0422
We had a different formula for double root.0433
The general solution c1 x4 but we can not have c2 x4 because that would just be a copy of our first solution.0439
C2 x4 natural log of x, we got that straight from the lesson overview at the beginning.0449
Whenever you have that double root, that second solution you just multiply it up by natural log of x.0459
That is the end of that one but just to recap we noticed our descending powers of x.0467
X2, x, and a constant, that is what triggers you that it is an Euler equation.0473
Write down your α is the coefficient of first, β is the coefficient of the second one.0478
Plot those into our generic characteristic equation where you have an α -1 so that -7 turns into -8, factor it out.0483
Once you get a double root for r you know one of your solutions is x4, but the other solution, in order to get an independent solution you got to multiply it by natural log of x.0493
That is our second independent solution there.0503
Our next example here, again we have Euler equation, we can check that by noticing the descending powers of x, x2, x, and a constant.0508
We got the descending powers of x, we got an Euler equation.0519
α here is -1, β is 5, those are the values we are going to use in the characteristic equation.0522
R2 + α – 1r + β= 0, if α is -1, then α -1 is 2, β is still 5.0533
Now that thing does not factor so we are going to jump in the quadratic formula to solve that.0551
Remember the quadratic formula says –b (+ or -) square root of b2 - 4ac/2a.0557
Here our b is -2 so our- b is +2 (+ or -) b2 is -22 so that is 4.0573
4ac is 4 × 1 × 5=20, over 2a is 2, that is 2 (+ or -) 4 – 20 is -16.0584
The square root of -16 is 4i, I’m going to get complex roots here, that simplifies down 1 (+ or-) 2i.0599
Remember we have a generic solution formula when you have complex roots.0614
The generic solution formula, let me remind you what that was from the lesson overview, the beginning of class.0620
C1 xa × cos natural log xb + c2 xa × sin of natural log of xb.0627
You could also use your natural log rules and write this as b natural log x inside, that will be ok if you look that better.0648
The a and b here, they are not the a and b from the original equation so be careful about that.0655
The a and b come from the a (+ or -) π here, it is not the same as these a’s and b’s that we used in the quadratic formula, be very careful about that.0661
What we have here is our general solution, c1 xa, our a is 1, I just write x × cos of natural log of xb, b is 2 here,0676
So natural log of x2 + c2 x × sin of natural log of x2 and that is our solution.0690
Let us take a look and see how that worked out, we had our Euler equation because of those descending powers of x, x2, x, and a constant.0712
We read off our coefficients, α is -1 the coefficient of the x term, β is 5, we plug those into the characteristic equation.0721
Remember the subtlety where the characteristic equation you drop the α down by 1.0732
α -1 becomes -2 and β is 5, to solve that we have to go to our quadratic formula.0737
That simplifies down to 1 (+ or-) 2i and we use that as our a and b, not the a and b from the quadratic formula but the 1 and the 2 are a and b,0747
That we are going to plug into our generic solution for Euler equation when you have complex roots.0760
We plug in x1 here and we get (x cos log of x2) and (x sin log of x2) as our 2 independent solutions.0768
We put them together with constants to make our general solution.0779
For example 4, we got x2 y″ – 6xy′ – 12 y=00785
We check out first that this satisfies the properties of being Euler equation, those descending powers on x, (x2, x, and a constant), (x2, x1, x0).0793
Remember it got to fit that format exactly to be an Euler equation, if it does not fit that format then you are really out of luck, you got to use some other techniques which certainly be more complicated.0805
It is worth checking if something is an Euler equation if so, these things are real pretty quick to solve.0817
If not then you got to have to do something that is probably be much more lengthy.0823
Since this one does work, we read off our α as -6, our β is 12, and we set up our characteristic equation.0827
R2 + α – 1, r + β= 0, that is our squared.0837
α -1 is -7, r + 12=0, that is another easy one to factor, that is r-3 × r-4=0.0846
R is 3 or 4, so 2 distinct real roots that is the easiest situation for an Euler equation.0861
Right away I can write down my general solution it is just c1 x3 form that first root + c2 x4 from that second root.0871
Just like that we are done with that one.0884
Let me remind you of how that one worked out, we first check the powers x2, x1, x0.0893
That looks like an Euler equation so that means I can write down the coefficients.0900
α=-6, β=12, drop them right into my characteristic equation which has that shift to the α down by 1.0904
We get r2 - 7r that is α-1 + 12=0, factors nicely and gives me couple of roots.0914
Those roots become the exponents on x for the general solution.0923
On example 5 here, again we have an Euler equation because we recognized this descending power of x’s.0932
X2, x1,and x0 here, no x at all means x0 or you think of it as being a constant.0939
I can read off my coefficients, α is 5, β is 4, I’m going to set up my characteristic equation.0948
It always has a form r2 + α -1r + β=0.0958
Remember to shift that α by 1, that is the subtlety of Euler equations that we have not really seen anywhere else.0967
In this case the α is 5, we get r2 + 4 r + 4 =0, that first 4 here, this one right here, that comes from 5-1, it has nothing to do with β being 4 there.0973
That is easy to solve, that is r + 22=0, r=-2 and that is a double root.0988
Remember we have a special formula for one you have a double root of an Euler equation and that formula is, first you have x to that power, c1x to that power.1001
But then you can not have c2 × x to that power again because that would just be a copy of your first solution.1013
The way you get around that is you multiply on a natural log of x.1021
That is our general solution to that one.1028
Let us recap how that problem worked out, we recognized the descending powers x2, x1, x0, ok that means it is an Euler equation.1039
We identify our α as a coefficient of the x term, β is our coefficient of the constant term.1051
Then we go to our generic characteristic equation with an α -1 in it and we get r2 + 4r + 4, that is using α -1 to get that 4 right there.1059
That factors easily into r + 22 = 0 that turns into r=-2, that is a double root.1075
In case of a double root, our solution is just like with 2 distinct roots, we form x to that power, x-2.1086
For the second one, we can not just form x-2 because that would be a copy of our first solution.1096
We go x-2 natural log of x to get ourselves a distinct solution and we put a constant on each one.1101
On example 6, we got the differential equation x2 y″ – 3xy′ + 29y=0.1112
As before, look at this we got x2, x1, x0, that means it is an Euler equation so we can use what we have been learning in this lecture.1122
We are going to identify our α and our β, α is -3 here, make sure you include the negative, sometimes people just see the 3 here and say ok α is 3.1135
Of course that is going to lead you to disaster later on, do not forget those negatives if they are part of it.1145
β is 29, we go to our generic characteristic equation r2 + α – 1 r + β =0.1152
α is -3, α -1 is -4, r + 29 =0 and it will be great if that would factor but it does not factor easily so we are going to the quadratic formula for that.1166
R=-b (+or -) the square root of b2 - 4ac / 2a.1185
In this case our b is -4 so –b is +4, (+ or -), b2 is 16 and 4ac is 4 × 1 × 29 which is 116, that is all divided by 2a but a is just 1 so that is 2.1196
That is 4 (+ or -) the square root of -100/2, now -100 the square root of that is 10i.1224
This is 4 (+ or -) 10i/2, 2 (+ or -) 5i and we have a generic solution formula for when we get complex roots to the characteristic equation.1237
It is c1 xa × cos of natural log of xb + c2 xa × sin of natural log of xb.1256
You could also write that as b natural log of x, that would be correct.1273
The a and b, they are not the a and b from back here in the quadratic formula, they are the a and b that you got in the end.1279
Let me go ahead and plug those in, the general solution here is (c1 × x2),( cos r of natural log5 + c2 x 2 × sin of natural log of x5.1290
You could write that as 5 natural log of x if you like.1312
That is our general solution to this Euler equation.1319
Let us go back and see how that worked out, first thing to do is recognize the powers, x2, x1,and x0.1329
That is what you have to have for an Euler equation to work out as those descending powers of x’s.1337
If you do its going to work out easily, if you do not you have to abandon the Euler methods completely and you have to try something completely different.1343
We found that it worked out for this example, we identify our α is the coefficient of the x term, our β is the coefficient of the constant term.1355
We go back to the generic characteristic equation r2 + α – 1r + β = 0.1372
Our α is -3 so subtracting 1 from that is where this -4 came from, we got this quadratic equation that really did not factor nicely.1381
So we use the quadratic formula, we got a –number under the square root so we get complex numbers 2 (+ or -) 5i.1391
Then we drop those as our a and b, not the a and b from the quadratic formula but our a and b from the complex number we found.1400
We drop those in to our generic solution formula for Euler equation for complex roots, which is xa cos log b + xa sin log of xb.1409
We get (c1 x2 cos log of x5) (c2 x2 sin of log of x5).1423
That is our general solution to the differential equation.1431
That is the end of our lecture on Euler equations, by the way you might have come here looking for Euler methods which is actually something quite different.1436
That is something we are going to get in to a later lecture here on the differential equations lectures.1446
If you are looking for Euler methods here and this did not look at all like what you are expecting, just scroll through and look for a later lecture on Euler methods.1451
That is a numerical solution to differential equation and you will find that here on www.educator.com.1459
It is just that this was a specific lecture about Euler equations.1465
That wraps everything up here, this has been the Euler equations lecture in the differential equations series here on www.educator.com.1470
My name is Will Murray and I thank you very much for watching, bye.1479

Professor Murray
Euler Equations
Slide Duration:Table of Contents
1h 7m 21s
- Intro0:00
- Lesson Objectives0:19
- How to Solve Linear Equations2:54
- Calculate the Integrating Factor2:58
- Changes the Left Side so We Can Integrate Both Sides3:27
- Solving Linear Equations5:32
- Further Notes6:10
- If P(x) is Negative6:26
- Leave Off the Constant9:38
- The C Is Important When Integrating Both Sides of the Equation9:55
- Example 110:29
- Example 222:56
- Example 336:12
- Example 439:24
- Example 544:10
- Example 656:42
35m 11s
- Intro0:00
- Lesson Objectives0:19
- Some Equations Are Both Linear and Separable So You Can Use Either Technique to Solve Them1:33
- Important to Add C When You Do the Integration2:27
- Example 14:28
- Example 210:45
- Example 314:43
- Example 419:21
- Example 527:23
1h 11m 36s
- Intro0:00
- Lesson Objectives0:20
- If You Can Manipulate a Differential Equation Into a Certain Form, You Can Draw a Slope Field Also Known as a Direction Field0:23
- How You Do This0:45
- Solution Trajectories2:49
- Never Cross Each Other3:44
- General Solution to the Differential Equation4:03
- Use an Initial Condition to Find Which Solution Trajectory You Want4:59
- Example 16:52
- Example 214:20
- Example 326:36
- Example 434:21
- Example 546:09
- Example 659:51
1h 5m 19s
- Intro0:00
- Lesson Overview0:38
- Mixing1:00
- Population2:49
- Finance3:22
- Set Variables4:39
- Write Differential Equation6:29
- Solve It10:54
- Answer Questions11:47
- Example 113:29
- Example 224:53
- Example 332:13
- Example 442:46
- Example 555:05
1h 1m 20s
- Intro0:00
- Lesson Overview0:18
- Autonomous Differential Equations Have the Form y' = f(x)0:21
- Phase Plane Analysis0:48
- y' < 02:56
- y' > 03:04
- If we Perturb the Equilibrium Solutions5:51
- Equilibrium Solutions7:44
- Solutions Will Return to Stable Equilibria8:06
- Solutions Will Tend Away From Unstable Equilibria9:32
- Semistable Equilibria10:59
- Example 111:43
- Example 215:50
- Example 328:27
- Example 431:35
- Example 543:03
- Example 649:01
28m 44s
- Intro0:00
- Lesson Overview0:36
- Linear Means0:50
- Second-Order1:15
- Homogeneous1:30
- Constant Coefficient1:55
- Solve the Characteristic Equation2:33
- Roots r1 and r23:43
- To Find c1 and c2, Use Initial Conditions4:50
- Example 15:46
- Example 28:20
- Example 316:20
- Example 418:26
- Example 523:52
31m 49s
- Intro0:00
- Lesson Overview0:15
- Sometimes The Characteristic Equation Has Complex Roots1:12
- Example 13:21
- Example 27:42
- Example 315:25
- Example 418:59
- Example 527:52
43m 2s
- Intro0:00
- Lesson Overview0:23
- If the Characteristic Equation Has a Double Root1:46
- Reduction of Order3:10
- Example 17:23
- Example 29:20
- Example 314:12
- Example 431:49
- Example 533:21
50m 1s
- Intro0:00
- Lesson Overview0:11
- Inhomogeneous Equation Means the Right Hand Side is Not 0 Anymore0:21
- First Solve the Homogeneous Equation1:04
- Find a Particular Solution to the Inhomogeneous Equation Using Undetermined Coefficients2:03
- g(t) vs. Guess for ypar2:42
- If Any Term of Your Guess for ypar Looks Like Any Term of yhom5:07
- Example 17:54
- Example 215:25
- Example 323:45
- Example 433:35
- Example 542:57
49m 22s
- Intro0:00
- Lesson Overview0:31
- Inhomogeneous vs. Homogeneous0:47
- First Solve the Homogeneous Equation1:17
- Notice There is No Coefficient in Front of y''1:27
- Find a Particular Solution to the Inhomogeneous Equation Using Variation of Parameters2:32
- How to Solve4:33
- Hint on Solving the System5:23
- Example 17:27
- Example 217:46
- Example 323:14
- Example 431:49
- Example 536:00
57m 38s
- Intro0:00
- Lesson Overview0:36
- Taylor Series Expansion0:37
- Maclaurin Series2:36
- Common Maclaurin Series to Remember From Calculus3:35
- Radius of Convergence7:58
- Ratio Test12:05
- Example 115:18
- Example 220:02
- Example 327:32
- Example 439:33
- Example 545:42
1h 20m 28s
- Intro0:00
- Lesson Overview0:49
- Guess a Power Series Solution and Calculate Its Derivatives, Example 11:03
- Guess a Power Series Solution and Calculate Its Derivatives, Example 23:14
- Combine the Series5:00
- Match Exponents on x By Shifting Indices5:11
- Match Starting Indices By Pulling Out Initial Terms5:51
- Find a Recurrence Relation on the Coefficients7:09
- Example 17:46
- Example 219:10
- Example 329:57
- Example 441:46
- Example 557:23
- Example 61:09:12
24m 42s
- Intro0:00
- Lesson Overview0:11
- Euler Equation0:15
- Real, Distinct Roots2:22
- Real, Repeated Roots2:37
- Complex Roots2:49
- Example 13:51
- Example 26:20
- Example 38:27
- Example 413:04
- Example 515:31
- Example 618:31
1h 26m 17s
- Intro0:00
- Lesson Overview0:13
- Singular Point1:17
- Definition: Pole of Order n1:58
- Pole Of Order n2:04
- Regular Singular Point3:25
- Solving Around Regular Singular Points7:08
- Indical Equation7:30
- If the Difference Between the Roots is An Integer8:06
- If the Difference Between the Roots is Not An Integer8:29
- Example 18:47
- Example 214:57
- Example 325:40
- Example 447:23
- Example 51:09:01
41m 52s
- Intro0:00
- Lesson Overview0:09
- Laplace Transform of a Function f(t)0:18
- Laplace Transform is Linear1:04
- Example 11:43
- Example 218:30
- Example 322:06
- Example 428:27
- Example 533:54
47m 5s
- Intro0:00
- Lesson Overview0:09
- Laplace Transform L{f}0:13
- Run Partial Fractions0:24
- Common Laplace Transforms1:20
- Example 13:24
- Example 29:55
- Example 314:49
- Example 422:03
- Example 533:51
45m 15s
- Intro0:00
- Lesson Overview0:12
- Start With Initial Value Problem0:14
- Take the Laplace Transform of Both Sides of the Differential Equation0:37
- Plug in the Identities1:20
- Take the Inverse Laplace Transform to Find y2:40
- Example 14:15
- Example 211:30
- Example 317:59
- Example 424:51
- Example 536:05
57m 30s
- Intro0:00
- Lesson Overview0:41
- Matrix0:54
- Determinants4:45
- 3x3 Determinants5:08
- Eigenvalues and Eigenvectors7:01
- Eigenvector7:48
- Eigenvalue7:54
- Lesson Overview8:17
- Characteristic Polynomial8:47
- Find Corresponding Eigenvector9:03
- Example 110:19
- Example 216:49
- Example 320:52
- Example 425:34
- Example 535:05
59m 26s
- Intro0:00
- Lesson Overview1:11
- How to Solve Systems2:48
- Find the Eigenvalues and Their Corresponding Eigenvectors2:50
- General Solution4:30
- Use Initial Conditions to Find c1 and c24:57
- Graphing the Solutions5:20
- Solution Trajectories Tend Towards 0 or ∞ Depending on Whether r1 or r2 are Positive or Negative6:35
- Solution Trajectories Tend Towards the Axis Spanned by the Eigenvector Corresponding to the Larger Eigenvalue7:27
- Example 19:05
- Example 221:06
- Example 326:38
- Example 436:40
- Example 543:26
- Example 651:33
1h 3m 54s
- Intro0:00
- Lesson Overview0:47
- Recall That to Solve the System of Linear Differential Equations, We find the Eigenvalues and Eigenvectors0:52
- If the Eigenvalues are Complex, Then They Will Occur in Conjugate Pairs1:13
- Expanding Complex Solutions2:55
- Euler's Formula2:56
- Multiply This Into the Eigenvector, and Separate Into Real and Imaginary Parts1:18
- Graphing Solutions From Complex Eigenvalues5:34
- Example 19:03
- Example 220:48
- Example 328:34
- Example 441:28
- Example 551:21
45m 17s
- Intro0:00
- Lesson Overview0:44
- If the Characteristic Equation Has a Repeated Root, Then We First Find the Corresponding Eigenvector1:14
- Find the Generalized Eigenvector1:25
- Solutions from Repeated Eigenvalues2:22
- Form the Two Principal Solutions and the Two General Solution2:23
- Use Initial Conditions to Solve for c1 and c23:41
- Graphing the Solutions3:53
- Example 18:10
- Example 216:24
- Example 323:25
- Example 431:04
- Example 538:17
43m 37s
- Intro0:00
- Lesson Overview0:35
- First Solve the Corresponding Homogeneous System x'=Ax0:37
- Solving the Inhomogeneous System2:32
- Look for a Single Particular Solution xpar to the Inhomogeneous System2:36
- Plug the Guess Into the System and Solve for the Coefficients3:27
- Add the Homogeneous Solution and the Particular Solution to Get the General Solution3:52
- Example 14:49
- Example 29:30
- Example 315:54
- Example 420:39
- Example 529:43
- Example 637:41
1h 8m 12s
- Intro0:00
- Lesson Overview0:37
- Find Two Solutions to the Homogeneous System2:04
- Look for a Single Particular Solution xpar to the inhomogeneous system as follows2:59
- Solutions by Variation of Parameters3:35
- General Solution and Matrix Inversion6:35
- General Solution6:41
- Hint for Finding Ψ-16:58
- Example 18:13
- Example 216:23
- Example 332:23
- Example 437:34
- Example 549:00
45m 30s
- Intro0:00
- Lesson Overview0:32
- Euler's Method is a Way to Find Numerical Approximations for Initial Value Problems That We Cannot Solve Analytically0:34
- Based on Drawing Lines Along Slopes in a Direction Field1:18
- Formulas for Euler's Method1:57
- Example 14:47
- Example 214:45
- Example 324:03
- Example 433:01
- Example 537:55
41m 4s
- Intro0:00
- Lesson Overview0:43
- Runge-Kutta is Know as the Improved Euler Method0:46
- More Sophisticated Than Euler's Method1:09
- It is the Fundamental Algorithm Used in Most Professional Software to Solve Differential Equations1:16
- Order 2 Runge-Kutta Algorithm1:45
- Runge-Kutta Order 2 Algorithm2:09
- Example 14:57
- Example 210:57
- Example 319:45
- Example 424:35
- Example 531:39
38m 22s
- Intro0:00
- Lesson Overview1:04
- Partial Derivative of u with respect to x1:37
- Geometrically, ux Represents the Slope As You Walk in the x-direction on the Surface2:47
- Computing Partial Derivatives3:46
- Algebraically, to Find ux You Treat The Other Variable t as a Constant and Take the Derivative with Respect to x3:49
- Second Partial Derivatives4:16
- Clairaut's Theorem Says that the Two 'Mixed Partials' Are Always Equal5:21
- Example 15:34
- Example 27:40
- Example 311:17
- Example 414:23
- Example 531:55
44m 40s
- Intro0:00
- Lesson Overview0:28
- Partial Differential Equation0:33
- Most Common Ones1:17
- Boundary Value Problem1:41
- Common Partial Differential Equations3:41
- Heat Equation4:04
- Wave Equation5:44
- Laplace's Equation7:50
- Example 18:35
- Example 214:21
- Example 321:04
- Example 425:54
- Example 535:12
57m 44s
- Intro0:00
- Lesson Overview0:26
- Separation of Variables is a Technique for Solving Some Partial Differential Equations0:29
- Separation of Variables2:35
- Try to Separate the Variables2:38
- If You Can, Then Both Sides Must Be Constant2:52
- Reorganize These Intro Two Ordinary Differential Equations3:05
- Example 14:41
- Example 211:06
- Example 318:30
- Example 425:49
- Example 532:53
1h 24m 33s
- Intro0:00
- Lesson Overview0:38
- Fourier Series0:42
- Find the Fourier Coefficients by the Formulas2:05
- Notes on Fourier Series3:34
- Formula Simplifies3:35
- Function Must be Periodic4:23
- Even and Odd Functions5:37
- Definition5:45
- Examples6:03
- Even and Odd Functions and Fourier Series9:47
- If f is Even9:52
- If f is Odd11:29
- Extending Functions12:46
- If We Want a Cosine Series14:13
- If We Wants a Sine Series15:20
- Example 117:39
- Example 243:23
- Example 351:14
- Example 41:01:52
- Example 51:11:53
47m 41s
- Intro0:00
- Lesson Overview0:22
- Solving the Heat Equation1:03
- Procedure for the Heat Equation3:29
- Extend So That its Fourier Series Will Have Only Sines3:57
- Find the Fourier Series for f(x)4:19
- Example 15:21
- Example 28:08
- Example 317:42
- Example 425:13
- Example 528:53
- Example 642:22
1 answer
Mon Dec 8, 2014 5:33 PM
Post by Harjinder Singh on December 8, 2014
Hi Dr. Murray,
I am working on a similar problem. However, the problem asks you to find two linearly independent solutions of the DE and compute the Wronskian. How would I proceed with that after finding the general equation?
Problem:
Find two linearly independent solutions of (2x^2)y" + 3xy' - y = 0 for x > 0 and compute their Wronskian.
I was able to get the following general solution:
y = (c1)(x^1/2) + (c2)(x^-1)
Can I just plugin some arbitrary values for c1 and c2 to get two separate solutions of y and then test them out for linear independence using the Wronskian? Or are the individual terms [c1*x^(1/2)] and [c2*x^-1] considered two separate solutions of the DE and that's all I need?
1 answer
Thu May 1, 2014 1:29 PM
Post by Khanh Nguyen on April 29, 2014
Hi mr. I could not open you video . That is on the Euler equation
Is there anything go wrong with the website?