10.3 SPACE CURVES
so we finally obtain
dˆb
ds=−τˆn. (10.14)Taking the dot product of each side withnˆ, we see that the torsion of a curve is
given by
τ=−nˆ·dˆb
ds.We may also define the quantityσ=1/τ, which is called theradius of torsion.
Finally, we consider the derivativednˆ/ds.Sincenˆ=ˆb׈twe havednˆ
ds=dbˆ
ds׈t+ bˆ×dˆt
ds
=−τnˆ×ˆt+ bˆ×κˆn=τˆb−κˆt. (10.15)In summary,ˆt,nˆandbˆand their derivatives with respect tosare related to oneanother by the relations (10.13), (10.14) and (10.15), theFrenet–Serret formulae,
dˆt
ds=κˆn,dnˆ
ds=τˆb−κˆt,dbˆ
ds=−τnˆ. (10.16)Show that the acceleration of a particle travelling along a trajectoryr(t)is given bya(t)=dv
dtˆt+v2
ρnˆ,wherevis the speed of the particle,ˆtis the unit tangent to the trajectory,nˆis its principal
normal andρis its radius of curvature.The velocity of the particle is given by
v(t)=dr
dt=
dr
dsds
dt=
ds
dtˆt,whereds/dtis the speed of the particle, which we denote byv,andˆtis the unit vector
tangent to the trajectory. Writing the velocity asv=vˆt, and differentiating once more
with respect to timet,weobtain
a(t)=dv
dt=
dv
dtˆt+vdˆt
dt;
but we note that
dˆt
dt
=
ds
dtdˆt
ds=vκnˆ=v
ρnˆ.Therefore, we have
a(t)=dv
dtˆt+v2
ρnˆ.This shows that in addition to an accelerationdv/dtalong the tangent to the particle’s
trajectory, there is also an accelerationv^2 /ρin the direction of the principal normal. The
latter is often called thecentripetalacceleration.