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Planck units

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In physics, Planck units are physical units of measurement defined exclusively in terms of five universal physical constants listed below, in such a manner that these five physical constants take on the numerical value of one when expressed in terms of these units. Planck units elegantly simplify particular algebraic expressions appearing in physical law. Originally proposed in 1899 by German physicist Max Planck, these units are also known as natural units because the origin of their definition comes only from properties of nature and not from any human construct. Planck units are only one system of natural units among other systems, but are considered unique in that these units are not based on properties of any prototype object, or particle (that would be arbitrarily chosen) but are based only on properties of free space. The constants that Planck units, by definition, normalize to 1 are the:

Each of these constants can be associated with at least one fundamental physical theory: c with special relativity, G with general relativity and Newtonian gravity, ħ with quantum mechanics, ε0 with electrostatics, and kB with statistical mechanics and thermodynamics. Planck units have profound significance for theoretical physics since they simplify several recurring algebraic expressions of physical law by nondimensionalization. They are particularly relevant in research on unified theories such as quantum gravity.

Planck units are often semi-humorously referred to by physicists as God's units. They eliminate anthropocentric arbitrariness from the system of units: some physicists argue that communication with extraterrestrial intelligence would have to use such a system of units to make common reference to scale. Unlike the meter and second, which exist as fundamental units in the SI system for historical reasons (in human history), the Planck length and Planck time are conceptually linked at a fundamental physical level.

Natural units help physicists to reframe questions. Frank Wilczek puts this succinctly:

...We see that the question [posed] is not, "Why is gravity so feeble?" but rather, "Why is the proton's mass so small?" For in Natural (Planck) Units, the strength of gravity simply is what it is, a primary quantity, while the proton's mass is the tiny number [1/(13 quintillion)]...

The strength of gravity is simply what it is and the strength of the electromagnetic force simply is what it is. The electromagnetic force operates on a different physical quantity (electric charge) than gravity (mass) so it cannot be compared directly to gravity. To note that gravity is an extremely weak force is, from the point-of-view of Planck units, like comparing apples to oranges. It is true that the electrostatic repulsive force between two protons (alone in free space) greatly exceeds the gravitational attractive force between the same two protons, and that is because the charge on the protons is approximately the Planck unit of charge but the mass of the protons is far, far less than the Planck mass.

Base Planck units

All systems of measurement feature base units: in the International System of Units (SI), for example, the base unit of length is the meter. In the system of Planck units, the Planck base unit of length is known simply as the Planck length, the base unit of time is the Planck time, and so on. These units are derived from the five dimensional universal physical constants of Table 1, in such a manner that these constants are eliminated from fundamental equations of physical law when physical quantities are expressed in terms of Planck units. For example, Newton's law of gravitation:

is equivalent to

Both equations are dimensionally consistent and equally valid in any system of units, but the second equation, with G missing, is relating only dimensionless quantities since any ratio of like-dimensioned quantity is a dimensionless quantity. If, by a shorthand convention, it is axiomatically understood that all physical quantities are expressed in terms of Planck units, the ratios above may be expressed simply with the symbols of physical quantity, without being scaled by their corresponding unit:

In order for this last equation to be valid (without G present), F, m1, m2, and r are understood to be the dimensionless numerical values of these quantities measured in terms of Planck units. This is why Planck units or any other use of natural units should be employed with care. Referring to G = c = 1, Paul Wesson wrote that, "Mathematically it is an acceptable trick which saves labour. Physically it represents a loss of information and can lead to confusion."[1]


Table 1: Fundamental physical constants
Constant Symbol Dimension Value in SI units with uncertainties[2]
Speed of light in vacuum c L T −1 299792458 m s−1 (exact)
Gravitational constant G L3 M−1 T −2 6.67428(67)×10−11 m3 kg−1 s−2
Reduced Planck constant ħ = h/2π, where h is the Planck constant L2 M T −1 1.054571628(53)×10−34 J s
Coulomb constant where ε0 is the permittivity of free space L3 M T −2 Q−2 8,987,551,787.368 1764 kg m3 s−2 C−2 (exact)
Boltzmann constant kB L2 M T −2 Θ−1 1.3806504(24)×10−23 J K−1

Key: L = length, M = mass, T = time, Q = electric charge, Θ = temperature. The exact values are due to the definitions of the metre and the ampere.


As can be seen above, the gravitational attractive force of two bodies of 1 Planck mass each, set apart by 1 Planck length is 1 Planck force. Likewise, the distance traveled by light during 1 Planck time is 1 Planck length. To determine, in terms of SI or other existing system of units, the quantitative values of the Planck units, those equations and three others must be satisfied to determine the five unknown quantities that define the Planck units:

Solving the five equations above for the five unknowns results in a unique set of values for the five base Planck units:

Table 2: Base Planck units Template:Base Planck units

Derived Planck units

In any system of measurement, units for many physical quantities can be derived from base units. Table 3 offers a sample of derived Planck units, some of which in fact are seldom used. As with the base units, their use is mostly confined to theoretical physics because most of them are too large or too small for empirical or practical use and there are large uncertainties in their values (see Discussion and Uncertainties in values below).

Table 3: Derived Planck units Template:Derived Planck units

Planck units simplify key equations

Physical quantities that have different dimensions (such as time and length) cannot be equated even if they are numerically equal (1 second is not the same as 1 metre). In theoretical physics, however, this scruple can be set aside, by a process called nondimensionalization. Table 4 shows how Planck units, by setting the numerical values of five fundamental constants to unity, nondimensionalizes and simplifies many fundamental equations of physics.

Table 4: How Planck units simplify the key equations of physics
Usual form Nondimensionalized form
Newton's law of universal gravitation
Einstein field equations in general relativity
Mass–energy equivalence in special relativity
Thermal energy per particle per degree of freedom
Boltzmann's entropy formula
Planck's relation for energy and angular frequency
Planck's law (surface intensity per unit solid angle per unit angular frequency) for black body at temperature T.
Stefan-Boltzmann constant σ defined
Bekenstein-Hawking black hole entropy[3]
Schrödinger's equation
Hamiltonian form of Schrödinger's equation
Covariant form of the Dirac equation
Coulomb's law
Maxwell's equations





Other possible normalizations

As already stated above, Planck units are derived by "normalizing" the numerical values of certain fundamental constants to 1. These normalizations are neither the only ones possible nor necessarily the best. Moreover, the choice of what factors to normalize, among the factors appearing in the fundamental equations of physics, is not evident, and the values of the Planck units are sensitive to this choice.

Possible alternative normalizations include:

Planck normalized to 1 the Coulomb force constant 1/(4πε0) (as does the cgs system of units). This sets the Planck impedance, ZP equal to Z0/4π, where Z0 is the characteristic impedance of free space. On the other hand, ε0 = 1:

The factor 4π is ubiquitous in theoretical physics because it equals the surface area of a unit sphere, and appears in the formulae for the surface area and volume of any three dimensional sphere. For example, gravitational and electrostatic fields produced by point charges have spherical symmetry (Barrow 2002: 214-15). The 4πr2 appearing in the denominator of Coulomb's law, for example, follows from the flux of an electrostatic field being distributed uniformly on the surface of a sphere. If space had more dimensions, the factor 4π would have to be changed.

In 1899, Newton's law of universal gravitation was still seen as fundamental, rather than as a convenient approximation holding for "small" velocities and distances, as general relativity was to inform us starting in 1915. Hence Planck normalized to 1 the gravitational constant G in Newton's law. In theories emerging after 1899, G nearly always appears multiplied by 4π or a small integer multiple thereof. Hence a fundamental choice that has to be made when designing a system of natural units is which, if any, instances of 4nπ appearing in the equations of physics are to be eliminated via the normalization. 4nπG = 1 for some value of n:

Hence a substantial body of physical theory discovered since Planck (1899) suggests normalizing to 1 not G but 4nπG, for one of n = 1, 2, or 4. However, doing so would introduce a factor of 1/(4nπ) into the nondimensionalized form of the law of universal gravitation.

Uncertainties in values

Planck units are clearly defined in terms of fundamental constants in Table 2 and yet, relative to other units of measurement such as SI, the values of those units are only known approximately. This is mostly due to uncertainty in the value of the gravitational constant G.

Today the value of the speed of light c in SI units is not subject to measurement error, because the SI base unit of length, the metre, is now defined as the length of the path travelled by light in vacuum during a time interval of 1/299 792 458 of a second. Hence the value of c is now exact by definition, and contributes no uncertainty to the SI equivalents of the Planck units. The same is true of the value of the vacuum permittivity ε0, due to the definition of ampere which sets the vacuum permeability μ0 to 4π × 10−7 H/m and the fact that μ0ε0 = 1/c2. The numerical value of the reduced Planck constant has been determined experimentally to 50 parts per billion, while that of G has been determined experimentally to no better than 1 part in 10000.[2] G appears in the definition of almost every Planck unit in Tables 2 and 3. Hence the uncertainty in the values of the Table 2 and 3 SI equivalents of the Planck units derives almost entirely from uncertainty in the value of G. (The propagation of the error in G is a function of the exponent of G in the algebraic expression for a unit. Since that exponent is ±12 for every base unit other than Planck charge, the relative uncertainty of each base unit is about one half that of G. This is indeed the case; according to CODATA, the experimental values of the SI equivalents of the base Planck units are known to about 1 part in 20,000.)

Discussion

Some Planck units are suitable for measuring quantities that are familiar from daily experience. For example:

However, most Planck units are many orders of magnitude too large or too small to be of any empirical and practical use, so that Planck units as a system are really only relevant to theoretical physics. In fact, 1 Planck unit is often the largest or smallest value of a physical quantity that makes sense given the current state of physical theory. For example:

  • A speed of 1 Planck length per Planck time is the speed of light in a vacuum, the maximum possible speed in special relativity;[5]
  • Our understanding of the Big Bang begins with the Planck Epoch, when the universe was 1 Planck time old and 1 Planck length in diameter, and had a Planck temperature of 1. At that moment, quantum theory as presently understood becomes applicable. Understanding the universe when it was less than 1 Planck time old requires a theory of quantum gravity that would incorporate quantum effects into general relativity. Such a theory does not yet exist;
  • At a Planck temperature of 1, all symmetries broken since the early Big Bang would be restored, and the four fundamental forces of contemporary physical theory would become one force.

Relative to the Planck Epoch, the universe today looks extreme when expressed in Planck units, as in this set of approximations (see, for example,[6] and [7]).

Table 5: Today's universe in Planck units.
Feature of present-day universe Approximate number of Planck units
Age 8.0 × 1060 tP (4.3 × 1017 seconds)
Diameter 5.4 x 1061 lP (8.7 × 1026 meters)
Mass Roughly 1060 mP (3 × 1052 kilograms, only counting stars); 1080 protons (sometimes known as the Eddington number)
Temperature 1.9 × 10−32 TP (temperature of the cosmic microwave background radiation, 2.725 kelvins)

The recurrence of the large number 1060 in the above table is a coincidence that intrigues some theorists. It is an example of the kind of large numbers coincidence that led theorists such as Eddington and Dirac to develop alternative physical theories. Theories derived from such coincidences are often dismissed by mainstream physicists as 'numerology'.

History

Natural units began in 1881, when George Johnstone Stoney derived units of length, time, and mass, now named Stoney units in his honor, by normalizing G, c, and the electron charge e to 1. (Stoney was also the first to hypothesize that electric charge is quantized and hence to see the fundamental character of e.) Max Planck first set out the base units (qP excepted) later named in his honor, in a paper presented to the Prussian Academy of Sciences in May 1899.[8][9] That paper also includes the first appearance of a constant named b, and later called h and named after him. The paper gave numerical values for the base units, in terms of the metric system of his day, that were remarkably close to those in Table 2. We are not sure just how Planck came to discover these units because his paper gave no algebraic details. But he did explain why he valued these units as follows:

...ihre Bedeutung für alle Zeiten und für alle, auch außerirdische und außermenschliche Kulturen notwendig behalten und welche daher als »natürliche Maßeinheiten« bezeichnet werden können... ...These necessarily retain their meaning for all times and for all civilizations, even extraterrestrial and non-human ones, and can therefore be designated as "natural units"...

Planck units and the invariant scaling of nature

Some theorists (such as Dirac and Milne) have proposed cosmologies that conjecture that physical "constants" might actually change over time (e.g. Dirac's Large Numbers Hypothesis). Such cosmologies have not gained mainstream acceptance and yet there is still considerable scientific interest in the possibility that physical 'constants' might change, although such propositions introduce many difficult questions. A few such questions that are relevant here might be: How would such a change make a noticeable operational difference in physical measurement or, more basically, our perception of reality? If some physical constant had changed, how would we notice it? How would physical reality be different? Which changed constants result in a meaningful and measurable differences? If a dimensionful physical constant such as the speed of light did change, would we be able to notice it? George Gamow argued in his book Mr. Tompkins in Wonderland that any change in a dimensionful physical constant, such as the speed of light in a vacuum, would result in obvious changes.

[An] important lesson we learn from the way that pure numbers like α define the world is what it really means for worlds to be different. The pure number we call the fine structure constant and denote by α is a combination of the electron charge, e, the speed of light, c, and Planck's constant, h. At first we might be tempted to think that a world in which the speed of light was slower would be a different world. But this would be a mistake. If c, h, and e were all changed so that the values they have in metric (or any other) units were different when we looked them up in our tables of physical constants, but the value of α remained the same, this new world would be observationally indistinguishable from our world. The only thing that counts in the definition of worlds are the values of the dimensionless constants of Nature. If all masses were doubled in value [including the Planck mass mP] you cannot tell because all the pure numbers defined by the ratios of any pair of masses are unchanged.

— Barrow 2002[10]

Referring to Michael Duff (Comment on time-variation of fundamental constants) and Duff, Okun, and Veneziano (Trialogue on the number of fundamental constants - The operationally indistinguishable world of Mr. Tompkins), if all physical quantities (masses and other properties of particles) were expressed in terms of Planck units, those quantities would be dimensionless numbers (mass divided by the Planck mass, length divided by the Planck length, etc.) and the only quantities that we ultimately measure in physical experiments or in our perception of reality are dimensionless numbers. When one commonly measures a length with a ruler or tape-measure, that person is actually counting tick marks on a given standard or is measuring the length relative to that given standard, which is a dimensionless value. It is no different for physical experiments, as all physical quantities are measured relative to some other like-dimensioned values.

We can notice a difference if some dimensionless physical quantity such as α or the proton/electron mass ratio changes (atomic structures would change) but if all dimensionless physical quantities remained constant (this includes all possible ratios of identically dimensioned physical quantity), we could not tell if a dimensionful quantity, such as the speed of light, c, has changed. And, indeed, the Tompkins concept becomes meaningless in our existence if a dimensional quantity such as c has changed, even drastically.

If the speed of light c, were somehow suddenly cut in half and changed to c2, (but with the axiom that all dimensionless physical quantities continuing to remain the same), then the Planck Length would increase by a factor of from the point-of-view of some unaffected "god-like" observer on the outside. Measured by "mortal" observers in terms of Planck units, the new speed of light would be remain as 1 new Planck length per 1 new Planck time - which is no different to the old measurement. But, since by axiom, the size of atoms (approximately the Bohr radius) are related to the Planck length by an unchanging dimensionless constant of proportionality:

Then atoms would be bigger (in one dimension) by , each of us would be taller by , and so would our meter sticks be taller (and wider and thicker) by a factor of . Our perception of distance and lengths relative to the Planck length is, by axiom, an unchanging dimensionless constant.

Our clocks would tick slower by a factor of (from the point-of-view of this unaffected "god-like" observer) because the Planck time has increased by but we would not know the difference (our perception of durations of time relative to the Planck time is, by axiom, an unchanging dimensionless constant). This hypothetical god-like observer on the outside might observe that light now travels at half the speed that it used to (as well as all other observed velocities) but it would still travel 299792458 of our new meters in the time elapsed by one of our new seconds ( continues to equal 299792458 m/s). We would not notice any difference.

This contradicts what George Gamow writes in his book Mr. Tompkins; there, Gamow suggests that if a dimension-dependent universal constant such as c changed, we would easily notice the difference. The disagreement is better thought of as the ambiguity in the phrase "changing a physical constant"; what would happen depends on whether (1) all other dimensionless constants were kept the same, or whether (2) all other dimension-dependent constants are kept the same. The second choice is a somewhat confusing possibility, since most of our units of measurement are defined in relation to the outcomes of physical experiments, and the experimental results depend on the constants. (The only exception is the kilogram.) Gamow does not address this subtlety; the thought experiments he conducts in his popular works assume the second choice for "changing a physical constant".

This unvarying aspect of the Planck-relative scale, or that of any other system of natural units, leads many theorists to conclude that a hypothetical change in dimensionful physical constants can only be manifest as a change in dimensionless physical constants. One such dimensionless physical constant is the fine-structure constant. There are some experimental physicists who think they have in fact measured a change in the fine structure constant[11] and this has intensified the debate about the measurement of physical constants. According to some theorists[12] there are some very special circumstances in which changes in the fine-structure constant can be measured as a change in dimensionful physical constants. Others however reject the possibility of measuring a change in dimensionful physical constants under any circumstance.[13] The difficulty or even the impossibility of measuring changes in dimensionful physical constants has led some theorists to debate with each other whether or not a dimensionful physical constant has any practical significance at all and that in turn leads to questions about which dimensionful physical constants are meaningful.[14]

See also

Notes

  1. ^ Wesson P. S. (1980) "The application of dimensional analysis to cosmology," Space Science Reviews 27: 117.
  2. ^ a b Fundamental Physical Constants from NIST
  3. ^ Also see Roger Penrose (1989) The Emperor's New Mind. Oxford Univ. Press: 340-41.
  4. ^ Chiao, Raymond Y. (2007) "Generation and detection of gravitational waves at microwave frequencies by means of a superconducting two-body system."
  5. ^ Feynman, R. P.; Leighton, R. B.; Sands, M. (1963). "The Special Theory of Relativity". The Feynman Lectures on Physics. Vol. 1 "Mainly mechanics, radiation, and heat". Addison-Wesley. pp. 15–9. LCCN 63-0 – 0.
  6. ^ John D. Barrow, 2002. The Constants of Nature; From Alpha to Omega - The Numbers that Encode the Deepest Secrets of the Universe. Pantheon Books. ISBN 0-375-42221-8.
  7. ^ Barrow, John D.; Tipler, Frank J. (1986). The Anthropic Cosmological Principle (1st ed.). Oxford University Press. ISBN 978-0-19-282147-8. LCCN 87028148.
  8. ^ Planck (1899), p. 479.
  9. ^ *Tomilin, K. A., 1999, "Natural Systems of Units: To the Centenary Anniversary of the Planck System," 287-96.
  10. ^ John D. Barrow, 2002. The Constants of Nature; From Alpha to Omega - The Numbers that Encode the Deepest Secrets of the Universe. Pantheon Books. ISBN 0-375-42221-8.
  11. ^ Webbe, J. K. et al. (1999) "Further evidence for cosmological evolution of the fine structure constant," Phys. Rev. Lett. 82: 884.
  12. ^ Paul C. Davies, T. M. Davis, and C. H. Lineweaver (2002) "Cosmology: Black Holes Constrain Varying Constants," Nature 418: 602.
  13. ^ Michael Duff (2002) "Comment on time-variation of fundamental constants."
  14. ^ Michael Duff, O. Okun and Gabriele Veneziano (2002) "Trialogue on the number of fundamental constants," Journal of High Energy Physics 3: 023.

References

Template:Planckunits