Action (physics) explained

Action
Unit:	joule-second
Otherunits:	J⋅Hz
Symbols:	S
Baseunits:	kg⋅m⋅s
Dimension:	M ⋅ L ^{2} ⋅ T ^{-1}

In physics, action is a scalar quantity that describes how the balance of kinetic versus potential energy of a physical system changes with trajectory. Action is significant because it is an input to the principle of stationary action, an approach to classical mechanics that is simpler for multiple objects.^[1] Action and the variational principle are used in Feynman's quantum mechanics^[2] and in general relativity.^[3] For systems with small values of action similar to the Planck constant, quantum effects are significant.

In the simple case of a single particle moving with a constant velocity (thereby undergoing uniform linear motion), the action is the momentum of the particle times the distance it moves, added up along its path; equivalently, action is the difference between the particle's kinetic energy and its potential energy, times the duration for which it has that amount of energy.

More formally, action is a mathematical functional which takes the trajectory (also called path or history) of the system as its argument and has a real number as its result. Generally, the action takes different values for different paths.^[4] Action has dimensions of energy × time or momentum × length, and its SI unit is joule-second (like the Planck constant h).^[5]

Introduction

Introductory physics often begins with Newton's laws of motion, relating force and motion; action is part of a completely equivalent alternative approach with practical and educational advantages.^[1] However the concept took many decades to supplant Newtonian approaches and remains a challenge to introduce to students.^[6]

Simple example

For a trajectory of a baseball moving in the air on Earth the action is defined between two points in time,

t _{1} and t _{2} as the kinetic energy minus the potential energy, integrated over time.^[7] S = \int ^{t _{2}} _{t _{1}} \left( KE(t) - PE(t)\right) dt The action balances kinetic against potential energy.^[7] The kinetic energy of a baseball of mass m is ( 1 / 2 )mv ^{2} where v is the velocity of the ball; the potential energy is mgx where g is the gravitational constant. Then the action between t _{1} and t _{2} isS = \int ^{t _{2}} _{t _{1}} \left( (1)/(2) m v ^{2(t)} - mg x(t) \right) dt The action value depends upon the trajectory taken by the baseball through x(t) and v(t) . This makes the action an input to the powerful stationary-action principle for classical and for quantum mechanics. Newton's equations of motion for the baseball can be derived from the action using the stationary-action principle, but the advantages of action-based mechanics only begin to appear in cases where the Newton's laws are difficult to apply. Replace the baseball by an electron: classical mechanics fails but stationary action continues to work.^[7] The energy difference in the simple action definition, kinetic minus potential energy, is generalized and called the Lagrangian for more complex cases.

Planck's quantum of action

The Planck constant, written as

h or \hbar when including a factor of 1 / 2 \pi , is called the quantum of action.^[8] Like action, this constant has unit of energy times time. It figures in all significant quantum equations, like the uncertainty principle and the de Broglie wavelength. Whenever the value of the action approaches the Planck constant, quantum effects are significant.^[7]

History

See main article: History of variational principles in physics. Pierre Louis Maupertuis and Leonhard Euler working in the 1740s developed early versions of the action principle. Joseph Louis Lagrange clarified the mathematics when he invented the calculus of variations. William Rowan Hamilton made the next big breakthrough, formulating Hamilton's principle in 1853.^[9] Hamilton's principle became the cornerstone for classical work with different forms of action until Richard Feynman and Julian Schwinger developed quantum action principles.^[10]

Definitions

Expressed in mathematical language, using the calculus of variations, the evolution of a physical system (i.e., how the system actually progresses from one state to another) corresponds to a stationary point (usually, a minimum) of the action. Action has the dimensions of [energy] × [time], and its SI unit is joule-second, which is identical to the unit of angular momentum.

Several different definitions of "the action" are in common use in physics.^{[11] [12]} The action is usually an integral over time. However, when the action pertains to fields, it may be integrated over spatial variables as well. In some cases, the action is integrated along the path followed by the physical system.

The action is typically represented as an integral over time, taken along the path of the system between the initial time and the final time of the development of the system:$$\backslash mathcal\; =\; \backslash int\_^\; L\; \backslash ,\; dt,$$where the integrand L is called the Lagrangian. For the action integral to be well-defined, the trajectory has to be bounded in time and space.

Action (functional)

l{S} which takes a function of time and (for fields) space as input and returns a scalar.^{[13] [14]} In classical mechanics, the input function is the evolution q(t) of the system between two times t₁ and t₂, where q represents the generalized coordinates. The action l{S}[ q (t)] is defined as the integral of the Lagrangian L for an input evolution between the two times:$$\backslash mathcal[\backslash mathbf\{q\}(t)]\; =\; \backslash int\_^\; L(\backslash mathbf(t),\backslash dot(t),t)\backslash ,\; dt,$$where the endpoints of the evolution are fixed and defined as q _{1} = q (t _{1} ) and q _{2} = q (t _{2} ) . According to Hamilton's principle, the true evolution q_true(t) is an evolution for which the action l{S}[ q (t)] is stationary (a minimum, maximum, or a saddle point). This principle results in the equations of motion in Lagrangian mechanics.

Abbreviated action (functional)

In addition to the action functional, there is another functional called the abbreviated action. In the abbreviated action, the input function is the path followed by the physical system without regard to its parameterization by time. For example, the path of a planetary orbit is an ellipse, and the path of a particle in a uniform gravitational field is a parabola; in both cases, the path does not depend on how fast the particle traverses the path.

The abbreviated action

l{S} _{0} (sometime written as W ) is defined as the integral of the generalized momenta,$$p\_i\; =\; \backslash frac,$$ for a system Lagrangian L along a path in the generalized coordinates q _{i} :$$\backslash mathcal\_0\; =\; \backslash int\_^\; \backslash mathbf\; \backslash cdot\; d\backslash mathbf\; =\; \backslash int\_^\; \backslash Sigma\_i\; p\_i\; \backslash ,dq\_i.$$where q _{1} and q _{2} are the starting and ending coordinates.According to Maupertuis' principle, the true path of the system is a path for which the abbreviated action is stationary.

Hamilton's characteristic function

When the total energy E is conserved, the Hamilton–Jacobi equation can be solved with the additive separation of variables:$$S(q\_1,\; \backslash dots,\; q\_N,\; t)\; =\; W(q\_1,\; \backslash dots,\; q\_N)\; -\; E\; \backslash cdot\; t,$$where the time-independent function W(q₁, q₂, ..., q_N) is called Hamilton's characteristic function. The physical significance of this function is understood by taking its total time derivative

$$\backslash frac\; =\; \backslash frac\; \backslash dot\; q\_i\; =\; p\_i\; \backslash dot\; q\_i.$$

This can be integrated to give

$$W(q\_1,\; \backslash dots,\; q\_N)\; =\; \backslash int\; p\_i\backslash dot\; q\_i\; \backslash ,dt\; =\; \backslash int\; p\_i\; \backslash ,dq\_i,$$

which is just the abbreviated action.

Action of a generalized coordinate

A variable J_k in the action-angle coordinates, called the "action" of the generalized coordinate q_k, is defined by integrating a single generalized momentum around a closed path in phase space, corresponding to rotating or oscillating motion:^[15]

$$J\_k\; =\; \backslash oint\; p\_k\; \backslash ,dq\_k$$

The corresponding canonical variable conjugate to J_k is its "angle" w_k, for reasons described more fully under action-angle coordinates. The integration is only over a single variable q_k and, therefore, unlike the integrated dot product in the abbreviated action integral above. The J_k variable equals the change in S_k(q_k) as q_k is varied around the closed path. For several physical systems of interest, J_k is either a constant or varies very slowly; hence, the variable J_k is often used in perturbation calculations and in determining adiabatic invariants. For example, they are used in the calculation of planetary and satellite orbits.^[15]

Single relativistic particle

See main article: Relativistic Lagrangian mechanics and Theory of relativity.

\tau is$$S\; =\; -\; m\; c^2\; \backslash int\_\; \backslash ,\; d\; \backslash tau.$$

If instead, the particle is parametrized by the coordinate time t of the particle and the coordinate time ranges from t₁ to t₂, then the action becomes$$S\; =\; \backslash int\_^\; L\; \backslash ,\; dt,$$where the Lagrangian is^[16] $$L\; =\; -mc^2\; \backslash sqrt.$$

Action principles and related ideas

See main article: Principle of stationary action.

Physical laws are frequently expressed as differential equations, which describe how physical quantities such as position and momentum change continuously with time, space or a generalization thereof. Given the initial and boundary conditions for the situation, the "solution" to these empirical equations is one or more functions that describe the behavior of the system and are called equations of motion.

Action is a part of an alternative approach to finding such equations of motion. Classical mechanics postulates that the path actually followed by a physical system is that for which the action is minimized, or more generally, is stationary. In other words, the action satisfies a variational principle: the principle of stationary action (see also below). The action is defined by an integral, and the classical equations of motion of a system can be derived by minimizing the value of that integral.

The action principle provides deep insights into physics, and is an important concept in modern theoretical physics. Various action principles and related concepts are summarized below.

Maupertuis's principle

See main article: Maupertuis's principle. In classical mechanics, Maupertuis's principle (named after Pierre Louis Maupertuis) states that the path followed by a physical system is the one of least length (with a suitable interpretation of path and length). Maupertuis's principle uses the abbreviated action between two generalized points on a path.

Hamilton's principal function

See main article: Hamilton's principle.

Hamilton's principle states that the differential equations of motion for any physical system can be re-formulated as an equivalent integral equation. Thus, there are two distinct approaches for formulating dynamical models.

Hamilton's principle applies not only to the classical mechanics of a single particle, but also to classical fields such as the electromagnetic and gravitational fields. Hamilton's principle has also been extended to quantum mechanics and quantum field theory—in particular the path integral formulation of quantum mechanics makes use of the concept—where a physical system explores all possible paths, with the phase of the probability amplitude for each path being determined by the action for the path; the final probability amplitude adds all paths using their complex amplitude and phase.^[17]

Hamilton–Jacobi equation

See main article: Hamilton–Jacobi equation. Hamilton's principal function

S = S(q,t;q _{0,t} _{0)} is obtained from the action functional l{S} by fixing the initial time t _{0} and the initial endpoint q _{0,} while allowing the upper time limit t and the second endpoint q to vary. The Hamilton's principal function satisfies the Hamilton–Jacobi equation, a formulation of classical mechanics. Due to a similarity with the Schrödinger equation, the Hamilton–Jacobi equation provides, arguably, the most direct link with quantum mechanics.

Euler–Lagrange equations

See main article: Euler–Lagrange equations.

In Lagrangian mechanics, the requirement that the action integral be stationary under small perturbations is equivalent to a set of differential equations (called the Euler–Lagrange equations) that may be obtained using the calculus of variations.

Classical fields

See also: Einstein–Hilbert action.

The action principle can be extended to obtain the equations of motion for fields, such as the electromagnetic field or gravitational field. Maxwell's equations can be derived as conditions of stationary action.

The Einstein equation utilizes the Einstein–Hilbert action as constrained by a variational principle. The trajectory (path in spacetime) of a body in a gravitational field can be found using the action principle. For a free falling body, this trajectory is a geodesic.

Conservation laws

See main article: Conservation laws.

Implications of symmetries in a physical situation can be found with the action principle, together with the Euler–Lagrange equations, which are derived from the action principle. An example is Noether's theorem, which states that to every continuous symmetry in a physical situation there corresponds a conservation law (and conversely). This deep connection requires that the action principle be assumed.

Path integral formulation of quantum field theory

See main article: Quantum mechanics and quantum field theory.

In quantum mechanics, the system does not follow a single path whose action is stationary, but the behavior of the system depends on all permitted paths and the value of their action. The action corresponding to the various paths is used to calculate the path integral, which gives the probability amplitudes of the various outcomes.

Although equivalent in classical mechanics with Newton's laws, the action principle is better suited for generalizations and plays an important role in modern physics. Indeed, this principle is one of the great generalizations in physical science. It is best understood within quantum mechanics, particularly in Richard Feynman's path integral formulation, where it arises out of destructive interference of quantum amplitudes.

Modern extensions

The action principle can be generalized still further. For example, the action need not be an integral, because nonlocal actions are possible. The configuration space need not even be a functional space, given certain features such as noncommutative geometry. However, a physical basis for these mathematical extensions remains to be established experimentally.

See also

• Calculus of variations
• Functional derivative
• Functional integral
• Hamiltonian mechanics
• Lagrangian
• Lagrangian mechanics
• Measure (physics)
• Noether's theorem
• Path integral formulation
• Principle of least action
• Principle of maximum entropy
• Some actions:
  • Nambu–Goto action
  • Polyakov action
  • Bagger–Lambert–Gustavsson action
  • Einstein–Hilbert action

Further reading

• The Cambridge Handbook of Physics Formulas, G. Woan, Cambridge University Press, 2010, .
• Dare A. Wells, Lagrangian Dynamics, Schaum's Outline Series (McGraw-Hill, 1967), A 350-page comprehensive "outline" of the subject.

External links

• Principle of least action interactive Interactive explanation/webpage

Notes and References

1. Neuenschwander . Dwight E. . Taylor . Edwin F. . Tuleja . Slavomir . 2006-03-01 . Action: Forcing Energy to Predict Motion . The Physics Teacher . en . 44 . 3 . 146–152 . 10.1119/1.2173320 . 0031-921X.
2. Ogborn . Jon . Taylor . Edwin F . 2005-01-01 . Quantum physics explains Newtons laws of motion . Physics Education . 40 . 1 . 26–34 . 10.1088/0031-9120/40/1/001 . 250809103 . 0031-9120.
3. Taylor . Edwin F. . 2003-05-01 . A call to action . American Journal of Physics . en . 71 . 5 . 423–425 . 10.1119/1.1555874 . 0002-9505.
4. Encyclopedia: Goodman . Bernard . Action . 1993. McGraw-Hill Encyclopaedia of Physics . McGraw-Hill . New York . Parker, S. P.. 0-07-051400-3. 22 . 2nd .
5. Encyclopedia: Stehle . Philip M. . Least-action principle . 1993. McGraw-Hill Encyclopaedia of Physics . McGraw-Hill . New York . Parker, S. P.. 0-07-051400-3. 670 . 2nd .
6. Fee . Jerome . 1942 . Maupertuis and the Principle of Least Action . American Scientist . 30 . 2 . 149–158 . 27825934 . 0003-0996.
7. Web site: The Feynman Lectures on Physics Vol. II Ch. 19: The Principle of Least Action . 2023-11-03 . www.feynmanlectures.caltech.edu.
8. Web site: Max Planck Nobel Lecture . live . https://web.archive.org/web/20230714164215/https://www.nobelprize.org/prizes/physics/1918/planck/lecture/ . 2023-07-14 . 2023-07-14.
9. Book: Kline, Morris. Mathematical Thought from Ancient to Modern Times. registration. Oxford University Press. New York. 1972. 167–168. 0-19-501496-0.
10. Book: Yourgrau . Wolfgang . Variational principles in dynamics and quantum theory . Mandelstam . Stanley . 1979 . Dover Publ . 978-0-486-63773-0 . Republ. of the 3rd ed., publ. in 1968 . Dover books on physics and chemistry . New York, NY.
11. Analytical Mechanics, L.N. Hand, J.D. Finch, Cambridge University Press, 2008,
12. Encyclopaedia of Physics (2nd Edition), R.G. Lerner, G.L. Trigg, VHC publishers, 1991, (Verlagsgesellschaft), (VHC Inc.)
13. The Road to Reality, Roger Penrose, Vintage books, 2007,
14. T. W. B. Kibble, Classical Mechanics, European Physics Series, McGraw-Hill (UK), 1973,
15. Book: Goldstein . Herbert . Classical mechanics . Poole . Charles P. . Safko . John L. . 2008 . Addison Wesley . 978-0-201-65702-9 . 3, [Nachdr.] . San Francisco Munich.
16. L. D. Landau and E. M. Lifshitz (1971). The Classical Theory of Fields. Addison-Wesley. Sec. 8. p. 24–25.
17. Quantum Mechanics, E. Abers, Pearson Ed., Addison Wesley, Prentice Hall Inc, 2004,