Uploaded by wpilads

2004 Chapter NewtonSAxioms

Newton’s Axioms
The Newtonian1 or classical mechanics is governed by three axioms, which are not independent of each other:
1. the law of inertia,
2. the fundamental equation of dynamics,
3. the interaction law,
and as a supplement: the theorems on independence concerning the superposition of forces
and of motions.
Premises of Newtonian mechanics are as follows:
1. The absolute time; that means that the time is the same in all coordinate frames, that
is, it is invariant: t = t . One may determine in any coordinate frame whether events
1 Isaac Newton, b. Jan. 4, 1643, Woolsthorpe (Lincolnshire)—d. March 31, 1727, London. Newton studied in
1660 at Trinity College in Cambridge, particularly with the eminent mathematician and theologian L. Barrow.
After getting various academic degrees and making a series of essential discoveries, in 1669 Newton became
successor of his teacher in Cambridge. In 1672 he was member and in 1703 president of the Royal Society. From
1688 to 1705, he was also member of Parliament, since 1696 attendant and since 1701 mint-master of the Royal
mint. Newton’s life’s work comprises, besides theological, alchemistic, and chronological-historical writings,
mainly works on optics and on pure and applied mathematics. In his investigations on optics he describes the
light as a flow of corpuscles and by this way interprets the spectrum and the composition of light, as well as the
Newton color rings, diffraction phenomena and double-refraction. His main opus Philosophiae Naturalis Principia
Mathematica (printed in 1687) is fundamental for the evolution of exact sciences. It includes the definition of the
most important basic concepts of physics, the three axioms of mechanics of macroscopic bodies, the principle
of “actio et reactio,” the gravitational law, the derivation of Kepler’s laws, and the first publication on fluxion
calculus. Newton also dealt with potential theory and with the equilibrium figures of rotating liquids. The ideas
for the great work emerged mainly in 1665–1666 when Newton had left Cambridge because of the pestilence.
In mathematics Newton worked on the theory of series, for example, in 1669 on the binomial series, on
interpolation theory, approximation methods, and the classification of cubic curves and conic sections. But
Newton could not remove logical problems even with his fluxion calculus that was represented in 1704 in detail.
His influence on the further development of mathematical sciences can hardly be judged, because Newton disliked
publishing. When Newton made his fluxion calculus public, his kind of treatment of problems of analysis was
already obsolete as compared to the calculus of Leibniz. The quarrel over whether Newton or Leibniz deserved
priority for developing the infinitesimal calculus continued until the 20th century. Detailed studies have shown
that they both obtained their results independently of each other [BR].
are simultaneous, because in classical physics one may imagine that signals are being
exchanged with infinitely large velocity.
2. The absolute space; that means that a coordinate frame, being at absolute rest, which
spans the full space, exists. This absolute space may be thought of as being represented
by the world ether, which shall be at absolute rest and so to speak embodies the absolute
space. Newton by himself did not believe in the ether; he could imagine the absolute space
also as being empty. In most recent time the 2.7 Kelvin radiation has been discovered.
This radiation is believed to originate from the Big Bang that presumably generated our
universe. A coordinate frame in which this radiation is isotropic—of equal intensity in
all directions—might also serve as such an absolute coordinate frame.
3. The mass being independent of the velocity.
4. The mass of a closed system of bodies (or mass points) is independent of the processes
going on in this system, no matter what kind these processes are.
The concepts of absolute time and absolute space, as well as the velocity independence of
the mass, are lost in the special theory of relativity. Finally, the fourth premise is no longer
fulfilled in high-energy processes as, for example, p + p → p + p + π + + π − . Here new
masses are generated.
Newton formulated his axioms essentially as follows:
Lex prima: Each body remains in its state of rest or uniform rectilinear motion as long
as it is not forced by acting forces to change this state.
Lex secunda: The change of motion is proportional to the effect of the driving force and
tends toward the direction of that straight line along which the force is acting.
Lex tertia: The action always equals the reaction, or the actions of two bodies onto each
other are always of equal magnitude and of opposite direction.
Lex quarta: Supplement to the laws of motion: Rule of the parallelogram of forces, that
is, forces add up like vectors. Thereby the superposition principle of the actions of forces
is postulated (principle of unperturbed superposition).
Because we deal in the following only with point mechanics, we have to introduce the
model representation of the mass point. Here one abstracts from shape, size, and rotational
motions of a body and considers only its translational motion. Newton’s axioms in modern
form then read as follows:
Axiom 1: Any mass point remains in the state of rest or rectilinear uniform motion until
this state is terminated by the action of other forces (i.e., by transfer of forces). This is a
special case of the second axiom. Namely,
F = 0,
m · v = constant.
Because of the presupposed velocity independece of the mass, it then holds that
v = constant.
If the “quantity of motion” p = m · v is denoted as the linear momentum of the mass point,
then the law of inertia is identical with the law of conservation of the linear momentum.
Axiom 2: The first time derivative of the linear momentum p of a mass point is equal to
the force F acting on it:
d(m · v)
= ṗ,
p = mv
is the linear momentum.2 .
Because in general the mass is a velocity-dependent quantity, that is, it is also timedependent, it must not simply be pulled in front of the bracket. In the nonrelativistic
Newtonian mechanics (v c ; c = 3 · 108 m s−1 ), the mass m is, however, treated as being
independent of the time, and one thus obtains the dynamic fundamental equation:
d 2r
= m 2 = m r̈ = ma.
That means that the acceleration a of a mass point is directly proportional to the force acting
on it and coincides with the direction of the force.
If several forces are acting simultaneously onto a mass point, then the above relation
according to the principle of superposition of forces reads
Fi .
Axiom 3: The forces exerted by two mass points onto each other have equal magnitude
and opposite directions; force = – counterforce:
Fi j = −F ji ,
where i = j.
Here Fi j is the force exerted by the jth point onto the ith point. F ji is the force exerted
by the ith onto the jth point.
Remark: The relation F = d(mv)/dt is on the one hand a definition of the force, on the
other hand a law. The statutory aspect is that, for example, the first time derivative of the
linear momentum occurs, but not the third or fourth or something else. Because the force
2 The time derivatives are often abbreviated with a dot, for example d f /dt ≡ f˙, v = dr/dt = ṙ, or a =
d 2 r/dt 2 = r̈ We will use this notation wherever it seems appropriate.
is the derivative of a vector with respect to a scalar (the time), it is a vector itself. Hence,
the addition of forces is governed, for instance, by the law of force parallelogram.
Problem 16.1:
Single-rope pulley
A weight W1 = M1 g hangs at the end of a rope. Here, g = 9.81 m/s2
is the gravitational acceleration of all bodies at the surface of the earth.
At the other end of the rope, hanging over a roller, a boy of weight
W2 = M2 g pulls himself upward. Let his acceleration relative to the
tightly mounted roller be a. What is the acceleration of the weight W1 ?
Let b be the acceleration of W1 and T the rope tension. The Newtonian
equations of motion then read
A boy and a weight hanging at the ends of a rope.
(a) For the mass M2 (boy):
−M2 · ae = M2 g e − T e;
(b) for the mass M1 (weight W1 ):
M1 b e = M1 g e − T e.
These are two equations with two unknowns (T, b). Their solution may be given immediately:
T = M2 (a + g);
(a + g)
(M1 − M2 )g − M2 a
If M1 = M2 , it follows that b = −a, as it should be. On the other hand, if a = 0, it follows that
b = (M1M−M
g and vanishes for the case M1 = M2 , as expected.
Problem 16.2:
Double-rope pulley
A mass M1 hangs at one end of a rope that is led over a roller A (compare the figure). The other end
carries a second roller of mass M2 , which in turn carries a rope with the masses m 1 and m 2 fixed to
its ends. The gravitational force is acting on all masses. Calculate the acceleration of the masses m 1
and m 2 , as well as the tensions T1 and T in the ropes.
We introduce the unit vector e ⊥ pointing upward (see figure)
and denote the string tensions by T = T e and T1 = T1 e,
respectively (see figure). The individual masses are influenced by the string tension (i.e., the force in the rope) and
by the gravitational force. We now write down the equations
of motion for the individual masses according to Newton’s
fundamental law.
M1 a1 e = −M1 ge + T e ,
m 1 (a2 − a1 )e = −m 1 ge + T1 e ,
m 2 (−a2 − a1 )e = −m 2 ge + T1 e .
−M2 a1 e = −M2 ge + T e − 2T1 e ,
The acceleration of the mass M1 has been denoted by a1 e,
that of the mass M2 is then (because of the constant rope
length) −a1 e; the acceleration of the mass m 1 relative to the Masses and forces at the doublemass M2 is a2 e, that of the mass m 2 is −a2 e. 16.5 represents rope pulley.
a set of four equations with the four unknowns: a1 , a2 , T, T1 .
Subtraction of the second equation from the first one yields
(M1 + M2 )a1 = −(M1 − M2 )g + 2T1 .
The addition of the last two equations of 16.5 leads to
−(m 1 + m 2 )a1 + (m 1 − m 2 )a2 = −(m 1 + m 2 )g + 2T1 .
The subtraction of 16.7 from 16.6 then yields a relation between a1 and a2 :
(M1 + M2 + m 1 + m 2 )a1 − (m 1 − m 2 )a2 = (−M1 + M2 + m 1 + m 2 )g .
A second relation of this kind is obtained by subtracting the last two equations 16.5 from each
other, namely
−(m 1 − m 2 )a1 + (m 1 + m 2 )a2 = −(m 1 − m 2 )g .
The accelerations a1 and a2 are now found from equations 16.8 and 16.9:
a1 =
−M1 (m 1 + m 2 ) + M2 (m 1 + m 2 ) + 4m 1 m 2
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
a2 =
−2M1 (m 1 − m 2 )
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
such that the total acceleration of mass m 1 is obtained as
a2 − a1 =
−M1 m 1 + 3M1 m 2 − M2 (m 1 + m 2 ) − 4m 1 m 2
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
and that of mass m 2 is
(−a2 − a1 ) =
M1 (3m 1 − m 2 ) − M2 (m 1 + m 2 ) − 4m 1 m 2
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
If all masses were identical (M1 = M2 = m 1 = m 2 ), then
a2 − a1 = − g,
a2 = 0,
−a2 − a1 = − g,
a1 = g,
as one would expect. The string tension T1 follows with 16.10 from equation 16.6 after a simple
calculation as
T1 =
(M1 + M2 )a1 + (M1 − M2 )g
4m 1 m 2 M1
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
The rope tension T is obtained from the first two equations 16.5, using 16.10 and 16.15, as
(M1 − M2 )a1
(M1 + M2 )g
+ T1
= M1 a1 + M1 g = M1 (a1 + g)
2(m 1 + m 2 )M1 M2 + 8m 1 m 2 M1
(m 1 + m 2 )(M1 + M2 ) + 4m 1 m 2
T =
According to 16.15 the rope tension T1 vanishes if one of the masses m 1 , m 2 , M1 vanishes. In this
case the rope is rolling without tension, as is clearly expected. The rope tension T vanishes if either
M1 = 0, or M2 and one of the masses m 1 or m 2 (or both) vanish. If m 1 = m 2 = m = 0 and if M1 = 0,
M2 = 0, a limit m → 0 can be taken:
T =
2M1 M2
M1 + M2
This is the rope tension in the case of the single roller with the two masses M1 and M2 at the rope