Physics Help
Special relativity
Special relativity
From Wikipedia, the free encyclopedia.
The special theory of relativity (SR) is the
physical theory published in
1905
by
Albert Einstein that modified
Newtonian physics to incorporate
electromagnetism as represented by
Maxwell's equations. The theory is called "special" because the theory
applies only to the special case of measurements made when both the observer and
that which is being observed are not affected by
gravity. Ten years later, Einstein published the theory of
General Relativity, or GR for short, which is the extension of special
relativity to incorporate gravitation.
Before the formulation of special relativity,
Hendrik Lorentz and others had already noted that electromagnetics differed
from Newtonian physics in that observations by one of some phenomenon can differ
from those of a person moving relative to that person at speeds nearing the
speed of light. For example, one may observe no
magnetic field, yet another observes a magnetic field in the same physical
area. Lorentz suggested an
aether theory in which objects and observers travelling with respect to a
stationary
aether underwent a physical shortening (Lorentz-Fitzgerald
contraction) and a change in temporal rate (time
dilation). This allowed the partial reconciliation of electromagnetics
and Newtonian physics. When the velocities involved are much less than speed of
light, the resulting laws simplify to Newton's laws. The theory, known as
Lorentz Ether Theory (LET) was criticized (even by Lorentz himself) because
of its ad
hoc nature.
While Lorentz suggested the
Lorentz transformation equations as a mathematical description that
accurately described the results of measurements, Einstein's contribution was to
derive these equations from a more fundamental theory. Einstein wanted
to know what was
invariant (the same) for all observers. His original title for his
theory was (translated from German) "Theory of Invariants". It was
Max Planck who suggested the term "relativity" to highlight the notion of
transforming the laws of physics between observers moving relative to
one another.
Special relativity is usually concerned with the behaviour of
objects and observers which remain at rest or are moving at a constant velocity.
In this case, the observer is said to be in an inertial frame of reference
or simply inertial. Comparison of the position and time of events as
recorded by different inertial observers can be done by using the Lorentz
transformation equations. A common misstatement about relativity is that SR
cannot be used to handle the case of objects and observers who are undergoing
acceleration (non-inertial reference frames), but this is incorrect.
For an example, see the
relativistic rocket problem. SR can correctly predict the behaviour of
accelerating bodies as long as the acceleration is not due to gravity, in which
case general relativity must be used.
SR postulated that the
speed of light in
vacuum is the same to all inertial observers, and said that every physical
theory should be shaped or reshaped so that it is the same mathematically for
every inertial observer. This postulate (which comes from Maxwell's equations
for electromagnetics) together with the requirement, successfully reproduces the
Lorentz transformation equations, and has several consequences that struck many
people as bizarre, among which are:
-
The time lapse between two events is not invariant from
observer to another, but is dependent on the relative speeds of the observers'
reference frames.
-
The
twin paradox is the "story" of a twin who flies off in a spaceship
travelling near the speed of light. When he returns he discovers that his twin
has aged much more rapidly than he has (or he aged more slowly).
-
Two events that occur simultaneously in different places in
one reference frame may occur one after the other in another reference frame
(relativity of
simultaneity).
-
The dimensions (e.g. length) of an object as measured by an
observer may differ from those by another.
-
The mass of a particle increases as it's velocity
increases. This led to the famous equation E = mc2. See below.
Another radical consequence is the rejection of the notion of
an absolute, unique, frame of reference. Previously it had been suggested that
the universe was filled with a substance known as "aether"
(absolute space), against which speeds could be measured. Aether had some
wonderful properties: it was sufficiently elastic that it could support
electromagnetc waves, those waves could interact with matter, yet it offered no
resistance to bodies passing through it. The results of various experiments,
culminating in the famous
Michelson-Morley experiment, suggested that either the Earth was always
stationary, or the notion of an absolute frame of reference was mistaken and
must be discarded.
Perhaps most far reaching, it also showed that
energy and
mass,
previously considered separate, were equivalent, and related by the most famous
expression from the theory:
-
E = mc2
where E is the energy of the body (at rest), m
is the mass and c is the speed of light. If the body is moving with
speed v relative to the observer, the total energy of the body is:
-
E = γmc2,
where
-
.
(The term γ occurs frequently in relativity, and comes from
the
Lorentz transformation equations.) It is worth noting that if v is
much less than c this can be written as
-
which is precisely equal to the "energy of existence", mc2,
and the Newtonian
kinetic energy, mv2/2. This is just one example of how
the two theories coincide when velocities are small.
At very high speeds, the denominator in the energy equation
(2) approaches a value of zero as the velocity approaches c. Thus, at
the speed of light, the energy would be infinite, which precludes things that
have mass from moving at that speed.
The most practical implication of this theory is that it puts
an upper limit to the laws (see
Law of nature) of
Classical Mechanics and
gravity formed by
Isaac Newton at the speed of light. Nothing carrying mass can move faster
than this speed. As an object's velocity approaches the speed of light, the
amount of energy required to accelerate it approaches infinity, making it
impossible to reach the speed of light. Only particles with no mass, such as
photons, can actually achieve this speed (and in fact they must always travel at
this speed in all frames of reference), which is approximately 300,000
kilometers per second or 186,300 miles per second.
The name "tachyon"
has been used for hypothetical particles which would move faster than the speed
of light, but to date evidence of the actual existence of tachyons has not been
produced.
Special relativity also holds that the concept of
simultaneity is relative to the observer: A 'time-like interval' has end-points
separated by a path along which it is possible for a hypothetical matter or
light to travel. A 'space-like interval' has end-points separated by a path in
space-time along which neither light nor any slower-than-light signal could
travel. No information can pass between points separated by a space-like
interval. Events along a space-like interval cannot influence one another by
transmitting light or matter, and would appear simultaneous to an observer in
the right frame of reference. To observers in different frames of reference,
event A could seem to come before event B or vice-versa; this does not apply to
events separated by time-like intervals.
Special relativity is now universally accepted by the physics
community, unlike
General Relativity which is still insufficiently confirmed by experiment to
exclude certain alternative theories of gravitation. However, there are a
handful of people opposed to relativity on various grounds and who have proposed
various alternatives, mainly
Aether theories. One alternative theory is
doubly-special relativity, where a characteristic length is added to the
list of invariant quantities.
SR uses a 'flat' 4 dimensional space, usually referred to as
space-time. This space, however, is very similar to the standard 3 dimensional
Euclidean space, and fortunately by that fact, very easy to work with.
The
differential of distance(ds) in cartesian 3D space is defined as:
-
where (dx1,dx2,dx3)
are the differentials of the three spatial dimensions. In the geometry of
special relativity, a fourth dimension, time, is added, with units of
c, so that the equation for the differential of distance becomes:
-
In many situations it may be convenient to treat time as
imaginary (e.g. it may simplify equations), in which case t in the
above equation is replaced by i.t', and the metric becomes
-
If we reduce the spatial dimensions to 2, so that we can
represent the physics in a 3-D space,
-
We see that the
null
geodesics lie along a dual-cone:
defined by the equation
-
, or
-
Which is the equation of a circle with r=c*dt. If we
extend this to three spatial dimensions, the null geodesics are continuous
concentric spheres, with radius = distance = c*(+ or -)time.
-
-
This null dual-cone represents the "line of sight" of a point
in space. That is, when we look at the stars and say "The light from that star
which I am receiving is X years old.", we are looking down this line of sight: a
null geodesic. We are looking at an event
meters away and d/c seconds in the past. For this reason the null dual
cone is also known as the 'light cone'. (The point in the lower left of the
picture below represents the star, the origin represents the observer, and the
line represents the null geodesic "line of sight".)
The cone in the -t region is the information that
the point is 'receiving', while the cone in the +t section is the
information that the point is 'sending'. We can envision a space of null
dual-cones:
and recall the concept of
cellular automata, applying it in a spatially and temporally continuous
fashion.
-
Michelson-Morley experiment - ether drift
-
Hamar experiment - obstruction of ether flow
-
Trouton-Noble experiment - torque on a capacitor
-
Kennedy-Thorndike experiment - time contraction
-
Forms of the emission theory experiment
Physics and Math:
Home | Up | Classical Mechanics | Thermodynamics | Statistical Mechanics | Electromagnetism | Special relativity General Relativity | Quantum Mechanics | Quantum Field Theory | Standard Model | Fluid Mechanics
Physics Help, made by MultiMedia | Free content and software
This guide is licensed under the GNU
Free Documentation License. It uses material from the Wikipedia.
|