4.2 Inertial and Gravitational Separations |
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And I am dumb to
tell a weather’s wind
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How time has ticked
a heaven round the stars.
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Dylan Thomas, 1934
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Special relativity, no less
than Galilean relativity, presupposes a three-dimensional space, within which
individual physical entities exist and move over time. Each localized entity
(such as a particle or a point of a field) has, at any given time, a position in
space that can be characterized by three real numbers, representing the spatial
coordinates of the entity, and all the spatial relations between entities can be
inferred from these coordinates. Hence, given N point-like entities, the
N(N-1)/2 spatial distances between pairs of entities (at a
given time) can be encoded as the 3N coordinates of those particles. From a
purely relational point of view, without presupposing any embedding in a
manifold with a fixed number of dimensions, we have no reason to expect such a
reduction in the degrees of freedom. Each of the N(N-1)/2 pair-wise separations
could be regarded as an independent quantity. The apparent fact that these
separations are not independent, but can be encoded in the form of N sets of
three numbers, which vary continuously with time, provides the justification for
the idea of particles moving in a coherent three-dimensional space, and is one
of the strongest arguments against the possibility of a purely relational basis
for physical theories – unless we include space (or spacetime) itself as a
dynamical entity.
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If we insist on a purely
relational theory, with no background space, one could argue that the
separations between entities ought to be regarded as the primary
ontological entities, with the particles serving merely abstract concepts to
organize our knowledge of those separations. The relationist view doesn’t even
presuppose a definite dimensionality of space, since each “separation” could be
considered to represent an independent degree of freedom, absent any additional
restricting principles. Of course, this freedom doesn’t seem to exist in the
real world, since (for example) we cannot arrange five particles all mutually
equidistant from each other. Nevertheless, it’s an interesting exercise to focus
on the spatial separations that exist between material particles, rather than on
the space and time coordinates of individual particles, to see if the behavior
of these separations can be characterized in a simple way.
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From the conventional point of
view, the simplest motion is that of a free particle moving inertially, i.e., in
a straight line at uniform speed, which can be described by saying that the
space coordinates are linear functions of the time coordinate (assuming a system
of inertial coordinates). From a relational standpoint, we consider the spatial
separation between two such particles. The three orthogonal components
Dx, Dy, and Dz of the separation are linear functions of time,
i.e.,
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where the coefficients
ai and bi are constants. Therefore the magnitude of any
such "co-inertial” separation is of the form
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where
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Letting the subscript n denote
nth derivative with respect to time, the first two derivatives of s(t)
are
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The right hand equation shows
that s2 s03 = k, and we can differentiate this
again and divide the result by s02 to show that the
separation s(t) between any two particles in relatively unaccelerated (i.e.,
co-inertial) motion in Galilean spacetime must satisfy the
equation
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Next, consider a particle of
mass m attached to a rod in such a way that it can slide freely along the rod.
If we rotate the rod about some fixed point, the particle will tend to slide
outward along the rod away from the center of rotation in accord with the basic
equation of motion
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where s is the distance from
the center of rotation to the sliding particle, and w is the angular velocity of the rod. Differentiating and
multiplying through by s0 gives
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Then since s2 =
w2s0, we see that s(t) satisfies the
equation
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which is formally similar to
(1).
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For a final example, consider
the separation between two massive particles in gravitational free-fall due to
their mutual gravitational attraction. Assume the two particles are identical,
each of mass m, lying along a line that is not rotating. According to Newtonian
theory the equation for this separation is
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where G is a universal
constant. Note that each particle's "absolute" acceleration is half of the
second derivative of their mutual separation with respect to time. Re-arranging
terms, we have s2 s02 = -2Gm. Differentiating this again and dividing through by
s0, we can characterize radial gravitational free-fall by the purely
kinematic equation
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So, we find once again that a
common (albeit idealized) class of physical separations satisfies the same form
of differential equation, even though in this case the separation is governed by
gravitation rather than just kinematics and inertia. All these separations are
characterized by an equation of the form
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for some constant N. (Among the
other solutions of this equation, with N = -1, are the elementary transcendental functions
et, sin(t), and cos(t). Solving for N, to isolate the arbitrary
constant, we have
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Differentiating both sides, we
get the basic equation
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If none of s0,
s1, s2, and s3 is zero, we can divide each term
by all of these to give the aesthetically appealing form
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This could be seen as a
(admittedly very simplistic) “unification” of a variety of physically meaningful
spatial separations under a single equation. However, this obviously doesn’t
encompass more than a tiny fraction of the variety of spatial separations in the
physical world. In fact, it’s clear that the objects of our experience, viewed
in isolation, cannot possibly be fully characterized by just their mutual
separations. For example, the separation between two massive particles, as
discussed above, beginning from a given stationary value, will shrink to zero
due to gravitational collapse, but only if the system of particles has no
angular momentum. If the particles are revolving about their common center of
mass at a suitable speed, the separation between them can remain constant. Thus
we have distinct outcomes for a single intrinsic configuration. This is similar
to Newton’s thought experiment with the rotating pail of water,
and it is another reason that Newton founded his
physics on the idea of absolute space, rather than on a purely relational basis.
Of course, as Mach observed, the evident physical effects of “absolute rotation”
don’t necessarily refute relationism as a viable basis for coordinating events.
It may be that we must take more relations into account. For example, even
though the two revolving particles are intrinsically identical to two stationary
particles, the configurations are distinct when the relations of the particles
to surrounding objects are considered. From this point of view, we wouldn’t
expect to be able to treat individual separations, or even a limited cluster of
related separations, in isolation. It would presumably be necessary to account
for all separations in the universe in order to correctly analyze any part of
the universe. This might seem to make relationism hopeless, but most attempts to
construct such a theory have invoked simplifying assumptions about the aggregate
effects of very distant separations.
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Newton’s achievement was finding a way to analyze isolated
parts of the world without having to explicitly refer to the rest of the
universe. All the effects of the distant universe can be encoded in the simple
concept of inertia in absolute space and time. To illustrate this approach, and
to show how it relates to the separation equation discussed above, consider the
general Newtonian equation of motion of a particle in a stationary spherical
gravitational field:
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In these equations, r is the
magnitude of the distance of the particle from the center of the field and
w is the absolute angular velocity of the
particle. A single coherent system of coordinates, with a single definition of
absolute rotation, suffices for the analysis of all physical systems. We have no
right to expect this to be true, but our experience has taught us that it is
true. Now, if we solve the left hand equation for w and differentiate to give dw/dt, we can substitute these expressions into the right
hand equation and re-arrange the terms to give
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which applies (in the Newtonian
limit) to arbitrary free paths of test particles in a gravitational field.
Obviously if m = 0 this reduces to equation (1), representing free inertial
separations, whereas for purely radial motion we have
d2r/dt2 = -m/r2, so this reduces to equation (3),
representing radial gravitational separation.
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Incidentally, even though the
above has been based on the Galilean spatial separations between objects as a
function of Galilean time, the same conditions can be shown to apply to the
absolute spacetime intervals between inertial particles as a function of their
proper times. Relative to any point on the worldline of one particle, the four
components Dt, Dx, Dy, and Dz of the absolute interval to any other inertially
moving particle are all linear functions of the proper time t along the latter particle's worldline. Therefore, the
components can be written in the form
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where the coefficients
ai and bi are constants. It follows that the absolute
magnitude of any "co-inertial separation" is of the form
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where
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Thus we have the same formal
dependence as before, except now the parameter s represents the absolute
spacetime separation. This shows that the absolute separation between any fixed
point on one inertial worldline and a point advancing along any other inertial
worldline satisfies equation (1), where subscripts denote derivatives with
respect to proper time of the advancing point. Naturally the reciprocal relation
also holds, as well as the absolute separation between two points, each
advancing along arbitrary inertial worldlines, correlated according to their
respective proper times.
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Friday, January 11, 2013
sr01 4.2 Inertial and Gravitational Separations
http://mathpages.com/rr/s4-02/4-02.htm
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