Imágenes de páginas
PDF
EPUB

the num

(n-1) (n-2) 2

[ocr errors]

It is obvious that when there exist n variables, ber of independent equations of condition is being the number of ways of equating two partial differential coefficients in a system in which n−1 are contained.

The solution of any such equation may be effected by an extension of the method adopted for equations with three variables. We must integrate as if all but two of the variables were constant, adding, in the place of an arbitrary constant, an arbitrary function of the variables which remain. This function we must determine by differentiating with respect to all the variables, and comparing with the equation given. If a single primitive exist, such determination will be possible. If a single primitive do not exist, we must, following the analogy of the corresponding case of three variables, endeavour to express the solution by a system of simultaneous equations. And such is indeed its general form. Pfaff, in a memoir published by the Berlin Academy 1814-15, has shewn that, according as the number of variables is 2n or 2n+1, the number of integral equations is n or n + 1 at most. His method, which is remarkable, consists of alternate integrations and transformations. For important commentaries and additions see Jacobi (Werke, Tom. I. p. 140), and Raabe (Crelle, Tom. XIV. p. 123).

Ex. Given (2x+y2+2xy,—y1)dx+2xydy-xdy,+x2dy,=0.

2

If we suppose the variables y1, y2, constant, we have to integrate

(2x + y2+ 2xy, −y1) dx + 2xydy = 0,

which, on substituting an arbitrary function of y,, y, represented by p, for an arbitrary constant, gives

[ocr errors]

Differentiating with respect to all the variables, we have

[ocr errors]

(2x + y2 + 2xy, −y1) dx + 2xydy — xdy1 + x2dy

[blocks in formation]
[merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][ocr errors][merged small]

Had we begun by making x and y constant, we should have had as the result of the first integration,

[ocr errors][merged small]

х

(b),

denoting a function of x and y. Differentiating with respect to all the variables and comparing with the given equation, we should find

[merged small][merged small][merged small][merged small][ocr errors]

the substitution of which in (b) reproduces the former solution (a).

Equations of an order higher than the first.

10. When an equation of the form

Adx2 + Bdy2 + Cdz2 +2Ddy dz + 2Edxdz +2Fdxdy = 0...(28) is resolvable into two equations each of the form

Pdx+Qdy + Rdz = 0,

the solution of either of these obtained by previous methods, will be a particular solution of (28), and the two solutions. taken disjunctively will constitute the complete solution, which is therefore expressed by the product of the equations of these solutions, each reduced to the form V= 0.

The condition under which (28) is resolvable as above, is expressed by the equation

ABC+2DEF-AD-BE- CF2 = 0......... (29).

B. D. E.

19

1

This is shewn by solving (28) with respect to dx, and assuming the quantity under the radical to be a complete square.

Forth & Thus, the equation a'da"+y'dy" — z'dz" + 2xy dx dy = 0,

which will be found to satisfy the above condition, is resolvable into the two equations

xdx+ydy+zdz = 0,

whence a2+y+z2 = c... (a),

xd + ydy – zdz=0,

x2 + y2 - z2 = c' ......(b).

Geometrically the solution is expressed by lines drawn in any manner on the surface, either of the sphere (a), or of the hyperboloid (b).

When the condition (29) is not satisfied, the proposed equation does not admit of a single primitive, or of any disjunctive system of primitives. But it does in general admit of a solution expressed by a system of simultaneous equations. Thus, if we integrate the equation dz2=m* (dx+dy), supposing a constant, we find z = my+ C, or, replacing C by a function of x,

z= my + $(x)

(c).

On substitution and integration, we find that this will satisfy the proposed equation if we have

[blocks in formation]

the system (c) (d) will therefore constitute a solution of the equation given. We enter not into the question whether it is the most general solution or not, proposing merely to exemplify the kind of solution of which the equation admits.

To this we may add that all equations which do not satisfy the conditions of integrability, though they may present themselves in the form of ordinary, have a far more intimate connexion with partial differential equations; and that this connexion affords the best clue to the solution of their theoretical difficulties.

[blocks in formation]

2. (x-3y-z) dx + (2y −3x) dy + (z − x) dz = 0.

3. (y + z) dx+(z+x) dy + (x + y) dz = 0.✔

4. yz dx + zx dy + xy dz = 0.

5. (y + z) dx + dy+dz=0. √

[blocks in formation]

7. (x2y—y3 — y3z) dx + (xy3 — x2z − x3) dy+ (xy2+ x2y) dz =0.

8. (2x2+2xy + 2xz2 + 1) dx + dy + 2zdz=0. ✓

9. (2x + y2+ 2xz) dx + 2xy dy – dw+x2 dz = 0.

10. Is the equation (1 + 2m) xdx + y (1 − x) dy + zdz= 0 derivable from a single primitive of the form p (x, y, z) = c? Foryst

11. Shew that any system of lines described on the surface of the sphere x2+ y2+ z2 = r2, and satisfying the above equation, would be projected on the plane xy in parabolas.

1.288, Ex-13

12. Shew that Monge's method would, if we integrate first with respect to a and z, present the solution of the equa-p

tion of Ex. 10, in the form

(1 + 2m) x2 + z2 = $(y), 2y (1-x) = − &′ (y).

13. Applying this form to the problem of Ex. 11, form and solve the differential equation for the determination of (y), and shew that it leads to the result stated in that Example.

14. Find the equation of the projections of the same system of curves on the plane yz.

Ex.14.

CHAPTER XIII.

SIMULTANEOUS DIFFERENTIAL EQUATIONS.

1. WE have hitherto considered only single differential equations. We have now to treat of systems of differential equations.

Of such by far the most important class is that in which one of the variables is independent and the others are dependent upon it, the number of equations in the system being equal to the number of dependent variables. Thus in the chief problem of physical astronomy-the problem of the motion of a system of material bodies abandoned to their mutual attractions-there is but one independent variable, the time; the dependent variables are the co-ordinates, which, varying with the time, determine the varying positions of the several members of the material system; while, lastly, the number of equations being equal to the number of co-ordinates involved, the dependence of the latter upon the time is made determinate.

Such a system of equations may properly be called a determinate system

We propose in this Chapter to treat only of systems of equations of the above class. And in the first instance we shall speak of simultaneous differential equations of the first order and degree, beginning with particular examples, and proceeding to the consideration of their general theory.

Particular Illustrations.

2. The simplest class of examples is that in which the equations of the given system are separately integrable. Fory, p.278, Ex. 1. Given ldx+mdy+ndz = 0, xdx+ydy+zdz = 0. Integrating separately, we have

[ocr errors]

lx+my+nz = c, x2 + y2+z2 = c';

and these equations expressing the complete solution of the given system may be said to constitute the primitive system.

« AnteriorContinuar »