Home

QuantumRelativity.com
Classical Electromagnetism
Appendix 3: Differential Equations
by Mark Lawrence

Football
Investing
Motorcycles
Neural Networks


Home

Articles
Calculus
Electromagnetism
Relativity
Physical Units
Space-Time Part I:
  Curved Space-Time
Space-Time Part II:
  Black Holes

References

Links

Art

Quotes

Recipes
Meat Marinades
Al Pastor
Carnitas
Frijoles: Refried Beans
Shrimp Burritos
Shrimp Enchiladas
Spanish Rice

Cioppino
Calzone or Pizza

Korma Chicken
Kung Pao Shrimp
Thai Chicken and Bamboo

Killer Shrimp
Seafood Chowder
Salmon
Grilled Shrimp
Spicy Tuna Herb Salad

Wisconsin Bratwurst
Cole Slaw
Soup with Dumplings
Garlic Cheese Sauce
Hot Garlic Butter
Greek Salad
Leg of Lamb

Cornbread
Chocolate Fruit & Nut Pie
Chocolate Truffles
Rice Pudding
Quick Chocolate Sauce
Quick Chocolate Pie

Cups-tsp-tbl-ml

Ant Killer

I recommend FireFox

A Basic Introduction to Differential Equations

Differential equations come up all the time in physics. This appendix can be considered a review / primer. It's not a substitute for a proper course.

Like integrals, differential equations are solved mostly by guessing. Unfortunately, there is little in the way of hard and fast rules. When we're solving a differential equation, we're looking for some function, F, that fits some particular prescription. The simpliest differential equation is:

d F
--- = 0
d x

This differential equation has as its only solution F(x) = constant. You can see this solution works by plugging the function into the equation and checking.

This differential equation is called a 1st order equation - there's only 1st order derivatives. Like polynomials, we're looking for as many solutions as there are orders. When we find that many solutions, we're done: the complete solution to the differential equation is the weighted sum of the seperate solutions.

The next simpliest differential equation is

d F
--- = k
d x

This equation has as its solution F = kx + c. Again, you can plug this in and try it out.

Next,

d F
--- = F
d x

That is, the derivative of the function is the function. We recognize the answer to this, F = ex. There's no rule that makes this obvious; we just remember, in exactly the same way we remember things when we do a crossword puzzle.

A very important pair of differential equations are:
 
d2F
---- = k2F
dx2
d2F
---- = -k2F
dx2

These second-order equations come up in physics all the time. It's important to recognize them instantly and see the various solutions instantly. The solution to the first equation is F = aekx + be-kx. These solutions have the rather unfortunate property that they're neither manifestly symmetric nor anti-symmetric. This can be easily fixed, however. Any function F(x) can be resolved into a symmetric and an anti-symmetric part,

Fsymmetric = ( F(x) + F(-x) ) / 2

Fanti-symmetric =  ( F(x) - F(-x) ) / 2

F = Fsymmetric + Fanti-symmetric

We can play the same trick with the solutions to the differential equation above,

Fsymmetric = (ekx + e-kx) / 2 = cosh( kx )

Fanti-symmetric =  = (ekx - e-kx) / 2 = sinh( kx )

Now our solutions will be F = a cosh( kx ) + b sinh( kx ).

The solution to the second equation is  F = aeikx + be-ikx. Again, these solutions are neither manifestly symmetric nor anti-symmetric. We can fix this with the same trick,

Fsymmetric = (eikx + e-ikx) / 2 = cos( kx )

Fanti-symmetric =  = (eikx - e-ikx) / 2i = sin( kx )

Now our solutions will be F = a cos( kx ) + b sin( kx ).
 
 


Copyright © 2002-2005 Mark Lawrence. All rights reserved. Reproduction is strictly prohibited.

Email me, mark@calsci.com, with suggestions, additions, broken links.
Revised Tuesday, 01-Mar-2005 12:10:00 PST