Bioche's rules

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Bioche's rules, formulated by the French mathematician Template:Ill (1859–1949), are rules to aid in the computation of certain indefinite integrals in which the integrand contains sines and cosines.

In the following, f(t) is a rational expression in sin⁡t and cos⁡t. In order to calculate ∫f(t)dt, consider the integrand ω(t)=f(t)dt. We consider the behavior of this entire integrand, including the dt, under translation and reflections of the t axis. The translations and reflections are ones that correspond to the symmetries and periodicities of the basic trigonometric functions.

Bioche's rules state that:

  1. If ω(−t)=ω(t), a good change of variables is u=cos⁡t.
  2. If ω(π−t)=ω(t), a good change of variables is u=sin⁡t.
  3. If ω(π+t)=ω(t), a good change of variables is u=tan⁡t.
  4. If two of the preceding relations both hold, a good change of variables is u=cos⁡2t.
  5. In all other cases, use u=tan⁡(t/2).

Because rules 1 and 2 involve flipping the t axis, they flip the sign of dt, and therefore the behavior of ω under these transformations differs from that of ƒ by a sign. Although the rules could be stated in terms of ƒ, stating them in terms of ω has a mnemonic advantage, which is that we choose the change of variables u(t) that has the same symmetry as ω.

These rules can be, in fact, stated as a theorem: one shows[1] that the proposed change of variable reduces (if the rule applies and if f is actually of the form f(t)=P(sin⁡t,cos⁡t)Q(sin⁡t,cos⁡t)) to the integration of a rational function in a new variable, which can be calculated by partial fraction decomposition.

Case of polynomials

To calculate the integral ∫sinp(t)cosq(t)dt, Bioche's rules apply as well.

  • If p and q are odd, one uses u=cos⁡(2t);
  • If p is odd and q even, one uses u=cos⁡(t);
  • If p is even and q odd, one uses u=sin⁡(t);
  • If not, one is reduced to lineariz.

Another version for hyperbolic functions

Suppose one is calculating ∫g(cosh⁡t,sinh⁡t)dt.

If Bioche's rules suggest calculating ∫g(cos⁡t,sin⁡t)dt by u=cos⁡(t) (respectively, sin⁡t,tan⁡t,cos⁡(2t),tan⁡(t/2)), in the case of hyperbolic sine and cosine, a good change of variable is u=cosh⁡(t) (respectively, sinh⁡(t),tanh⁡(t),cosh⁡(2t),tanh⁡(t/2)). In every case, the change of variable u=et allows one to reduce to a rational function, this last change of variable being most interesting in the fourth case (u=tanh⁡(t/2)).

Examples

Example 1

As a trivial example, consider

∫sin⁡tdt.

Then f(t)=sin⁡t is an odd function, but under a reflection of the t axis about the origin, ω stays the same. That is, ω acts like an even function. This is the same as the symmetry of the cosine, which is an even function, so the mnemonic tells us to use the substitution u=cos⁡t (rule 1). Under this substitution, the integral becomes −∫du. The integrand involving transcendental functions has been reduced to one involving a rational function (a constant). The result is −u+c=−cos⁡t+c, which is of course elementary and could have been done without Bioche's rules.

Example 2

The integrand in

∫dtsin⁡t

has the same symmetries as the one in example 1, so we use the same substitution u=cos⁡t. So

dtsin⁡t=−dusin2t=−du 1−cos2t.

This transforms the integral into

∫−du1−u2,

which can be integrated using partial fractions, since 11−u2=12(11+u+11−u). The result is that

∫dtsin⁡t=−12ln⁡1+cos⁡t1−cos⁡t+c.

Example 3

Consider

∫dt1+βcos⁡t,

where β2<1. Although the function f is even, the integrand as a whole ω is odd, so it does not fall under rule 1. It also lacks the symmetries described in rules 2 and 3, so we fall back to the last-resort substitution u=tan⁡(t/2).

Using cos⁡t=1−tan2(t/2)1+tan2(t/2) and a second substitution v=1−β1+βu leads to the result

∫dt1+βcos⁡t=21−β2arctan⁡[1−β1+βtan⁡t2]+c.

References

Template:WikiversityTemplate:Reflist

  • Zwillinger, Handbook of Integration, p. 108
  • Stewart, How to Integrate It: A practical guide to finding elementary integrals, pp. 190−197.