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In
physics, the
Planck length, denoted
ℓP, is a unit of
length, equal to
1.616229(38)×10−35 metres. It is a
base unit in the system of
Planck units, developed by physicist
Max Planck. The Planck length can be defined from three
fundamental physical constants: the
speed of light in a vacuum, the
Planck constant, and the
gravitational constant.
Value
The Planck length
ℓP is defined as:
Solving the above will show the approximate equivalent value of this unit with respect to the meter:
, where
is the
speed of light in a vacuum,
G is the
gravitational constant, and
ħ is the
reduced Planck constant. The two digits enclosed by
parentheses are the estimated
standard error associated with the reported numerical value.
[1][2]
The Planck length is about 10
−20 times the diameter of a
proton. It can be defined using the radius of
Planck particle.
Measuring the Planck length
In 2017 it was suggested by E. Haug
[3]
that the Planck length can be indirectly measured independent of any
knowledge of Newton's gravitational constant with for example the use of
a
Cavendish apparatus.
Further, it seems like the error in the Planck length measures must be
exactly half of that in the measurement errors of the Newton's
gravitational constant. That is the error as measured in percentage
term, also known as the relative standard uncertainty. This is in line
with the relative standard uncertainty reported by
NIST, which for the gravitational constant is
and for the Planck length is
.
History
In 1899
Max Planck[4]
suggested that there existed some fundamental natural units for length,
mass, time and energy. These he derived using dimensional analysis only
using the Newton gravitational constant, the speed of light and the
Planck constant. The natural units he derived has later been known as:
the Planck length, the Planck mass, the Planck time and the Planck
energy.
Theoretical significance
The Planck length is the scale at which
quantum gravitational effects are believed to begin to be apparent, where interactions require a working theory of quantum gravity to be analyzed.
[5] The Planck area is the area by which the surface of a spherical
black hole increases when the black hole swallows one bit of
information.
[6]
The Planck length is sometimes misconceived as the
minimum length of spacetime, but this is not accepted by conventional physics, as this would require violation or modification of
Lorentz symmetry.
[5] However, certain theories of
loop quantum gravity do attempt to establish a minimum length on the scale of the Planck length, though not necessarily the Planck length itself
[5], or attempt to establish the Planck length as observer-invariant, known as
doubly special relativity.
[citation needed]
The strings of
string theory are modelled to be on the order of the Planck length.
[5][7] In theories of
large extra dimensions, the Planck length has no fundamental physical significance, and quantum gravitational effects appear at other scales.
[citation needed]
Planck length and Euclidean geometry
The
gravitational field performs zero-point oscillations, and the geometry
associated with it also oscillates. The ratio of the circumference to
the radius varies near the Euclidean value. The smaller the scale, the
greater the deviations from the
Euclidean geometry.
Let us estimate the order of the wavelength of zero gravitational
oscillations, at which the geometry becomes completely unlike the
Euclidean geometry. The degree of deviation
of geometry from Euclidean geometry in the gravitational field is determined by the ratio of the gravitational potential
and the square of the speed of light
:
. When
, the geometry is close to Euclidean geometry; for
, all similarities disappear. The energy of the oscillation of scale
is equal to
(where
is the order of the oscillation frequency). The gravitational potential created by the mass
, at this length is
, where
is the constant of universal gravitation. Instead of
, we must substitute a mass, which, according to Einstein's formula, corresponds to the energy
(where
). We get
. Dividing this expression by
, we obtain the value of the deviation
. Equating
, we find the length at which the Euclidean geometry is completely distorted. It is equal to Planck length
m. Here there is a
quantum foam.
Visualization
The
size of the Planck length can be visualized as follows: if a particle
or dot about 0.005 mm in size (which is the same size as a
small grain of silt) were magnified in size to be as large as the
observable universe,
then inside that universe-sized "dot", the Planck length would be
roughly the size of an actual 0.005 mm dot. In other words, a 0.005 mm
dot is halfway between the Planck length and the size of the observable
universe on a
logarithmic scale.
[8]
All said, the attempt to visualize to an arbitrary scale of a 0.005 mm
dot is only for a hinge point. With no fixed frame of reference for time
or space, where the spatial units shrink toward infinitesimally small
spatial sections and time stretches toward infinity, scale breaks down.
Inverted, where space is stretched and time is shrunk, the scale adjusts
the other way according to the ratio V-squared/C-squared (
Lorentz transformation).
[clarification needed]