Inphysics,potential energy is theenergy of an object or system due to the body's position relative to other objects, or the configuration of its particles. The energy is equal to the work done against any restoring forces, such as gravity or those in a spring.^[1]

Potential energy
In the case of abow and arrow, when the archer doeswork on the bow, drawing the string back, some of the chemical energy of the archer's body is transformed intoelastic potential energy in the bent limb of the bow. When the string is released, the force between the string and the arrow does work on the arrow. The potential energy in the bow limbs is transformed into thekinetic energy of the arrow as it takes flight.
Common symbols	PE,U, orV
SI unit	joule (J)
Derivations from other quantities	U =mgh (gravitational) U =⁠1/2⁠kx2 (elastic) U =⁠1/2⁠CV2 (electric) U = −m ⋅B (magnetic) U =$\int F(r)dr$

The termpotential energy was introduced by the 19th-century Scottish engineer and physicistWilliam Rankine,^[2][3][4] although it has links to the ancient Greek philosopherAristotle's concept ofpotentiality.

Common types of potential energy includegravitational potential energy, theelastic potential energy of a deformed spring, and theelectric potential energy of anelectric charge and anelectric field. The unit for energy in theInternational System of Units (SI) is thejoule (symbol J).

Potential energy is associated with forces that act on a body in a way that the totalwork done by these forces on the body depends only on the initial and final positions of the body in space. These forces, whose total work is path independent, are calledconservative forces. If the force acting on a body varies over space, then one has aforce field; such a field is described by vectors at every point in space, which is, in turn, called avector field. A conservative vector field can be simply expressed as the gradient of a certain scalar function, called ascalar potential. The potential energy is related to, and can be obtained from, this potential function.

There are various types of potential energy, each associated with a particular type of force. For example, the work of anelastic force is called elastic potential energy; work of the gravitational force is called gravitational potential energy; work of theCoulomb force is calledelectric potential energy; work of thenuclear force acting on thebaryoncharge is called nuclear potential energy; work ofintermolecular forces is called intermolecular potential energy. Chemical potential energy, such as the energy stored infossil fuels, is the work of the Coulomb force during rearrangement of configurations of electrons and nuclei in atoms and molecules. Thermal energy usually has two components: the kinetic energy of random motions of particles and the potential energy of their configuration.

Forces derivable from a potential are also calledconservative forces. Thework done by a conservative force is$${\displaystyle W=-\mathrm{\Delta }U,}$$ where${\displaystyle \mathrm{\Delta }U}$  is the change in the potential energy associated with the force. The negative sign provides the convention that work done against a force field increases potential energy, while work done by the force field decreases potential energy. Common notations for potential energy arePE,U,V, andE_p.

Potential energy is the energy by virtue of an object's position relative to other objects.^[5] Potential energy is often associated with restoringforces such as aspring or the force ofgravity. The action of stretching a spring or lifting a mass is performed by an external force that works against the force field of the potential. This work is stored in the force field, which is said to be stored as potential energy. If the external force is removed the force field acts on the body to perform the work as it moves the body back to the initial position, reducing the stretch of the spring or causing a body to fall.

Consider a ball whose mass ism dropped from heighth. The accelerationg of free fall is approximately constant, so the weight force of the ballmg is constant. The product of force and displacement gives the work done, which is equal to the gravitational potential energy, thus$${\displaystyle U_{\text{g}}=mgh.}$$ 

The more formal definition is that potential energy is the energy difference between the energy of an object in a given position and its energy at a reference position.

From around 1840 scientists sought to define and understand energy andwork.^[4]The term "potential energy" was coined byWilliam Rankine a Scottish engineer and physicist in 1853 as part of a specific effort to develop terminology.^[2] He chose the term as part of the pair "actual" vs "potential" going back to work byAristotle. In his 1867 discussion of the same topic Rankine describes potential energy as 'energy of configuration' in contrast to actual energy as 'energy of activity'. Also in 1867,William Thomson introduced "kinetic energy" as the opposite of "potential energy", asserting that all actual energy took the form of⁠1/2⁠mv². Once this hypothesis became widely accepted, the term "actual energy" gradually faded.^[3]

Potential energy is closely linked withforces. If the work done by a force on a body that moves fromA toB does not depend on the path between these points (if the work is done by a conservative force), then the work of this force measured fromA assigns a scalar value to every other point in space and defines ascalar potential field. In this case, the force can be defined as the negative of thevector gradient of the potential field.

If the work for an applied force is independent of the path, then the work done by the force is evaluated from the start to the end of the trajectory of the point of application. This means that there is a functionU(x), called a "potential", that can be evaluated at the two pointsx_A andx_B to obtain the work over any trajectory between these two points. It is tradition to define this function with a negative sign so that positive work is a reduction in the potential, that is$${\displaystyle W={\int }_C\mathbf{F}\cdot d\mathbf{x}=U({\mathbf{x}}_{\text{A}})-U({\mathbf{x}}_{\text{B}})}$$ whereC is the trajectory taken from A to B. Because the work done is independent of the path taken, then this expression is true for any trajectory,C, from A to B.

The functionU(x) is called the potential energy associated with the applied force. Examples of forces that have potential energies are gravity and spring forces.

In this section the relationship between work and potential energy is presented in more detail. Theline integral that defines work along curveC takes a special form if the forceF is related to a scalar fieldU′(x) so that$${\displaystyle \mathbf{F}=\mathrm{\nabla }{U}^{\prime }=\left(\frac{\mathrm{\partial }{U}^{\prime }}{\mathrm{\partial }x},\frac{\mathrm{\partial }{U}^{\prime }}{\mathrm{\partial }y},\frac{\mathrm{\partial }{U}^{\prime }}{\mathrm{\partial }z}\right).}$$ This means that the units ofU′ must be this case, work along the curve is given by$${\displaystyle W={\int }_C\mathbf{F}\cdot d\mathbf{x}={\int }_C\mathrm{\nabla }{U}^{\prime }\cdot d\mathbf{x},}$$ which can be evaluated using thegradient theorem to obtain$${\displaystyle W=U^{\prime }({\mathbf{x}}_{\text{B}})-U^{\prime }({\mathbf{x}}_{\text{A}}).}$$ This shows that when forces are derivable from a scalar field, the work of those forces along a curveC is computed by evaluating the scalar field at the start point A and the end point B of the curve. This means the work integral does not depend on the path between A and B and is said to be independent of the path.

Potential energyU = −U′(x) is traditionally defined as the negative of this scalar field so that work by the force field decreases potential energy, that is$${\displaystyle W=U({\mathbf{x}}_{\text{A}})-U({\mathbf{x}}_{\text{B}}).}$$ 

In this case, the application of thedel operator to the work function yields,$${\displaystyle \mathrm{\nabla }W=-\mathrm{\nabla }U=-\left(\frac{\mathrm{\partial }U}{\mathrm{\partial }x},\frac{\mathrm{\partial }U}{\mathrm{\partial }y},\frac{\mathrm{\partial }U}{\mathrm{\partial }z}\right)=\mathbf{F},}$$ and the forceF is said to be "derivable from a potential".^[6] This also necessarily implies thatF must be aconservative vector field. The potentialU defines a forceF at every pointx in space, so the set of forces is called aforce field.

Given a force fieldF(x), evaluation of the work integral using thegradient theorem can be used to find the scalar function associated with potential energy. This is done by introducing a parameterized curveγ(t) =r(t) fromγ(a) =A toγ(b) =B, and computing, 

For the force fieldF, letv =dr/dt, then thegradient theorem yields, 

The power applied to a body by a force field is obtained from the gradient of the work, or potential, in the direction of the velocityv of the point of application, that is$${\displaystyle P(t)=-\mathrm{\nabla }U\cdot \mathbf{v}=\mathbf{F}\cdot \mathbf{v}.}$$ 

Examples of work that can be computed from potential functions are gravity and spring forces.^[7]

For small height changes, gravitational potential energy can be computed using$${\displaystyle U_{\text{g}}=mgh,}$$ wherem is the mass in kilograms,g is the local gravitational field (9.8 metres per second squared on Earth),h is the height above a reference level in metres, andU is the energy in joules.

In classical physics, gravity exerts a constant downward forceF = (0, 0,F_z) on the center of mass of a body moving near the surface of the Earth. The work of gravity on a body moving along a trajectoryr(t) = (x(t),y(t),z(t)), such as the track of a roller coaster is calculated using its velocity,v = (v_x,v_y,v_z), to obtain$${\displaystyle W={\int }_{t_1}^{t_2}\mathit{F}\cdot \mathit{v}dt={\int }_{t_1}^{t_2}{F}_{\text{z}}{v}_{\text{z}}dt=F_{\text{z}}\mathrm{\Delta }z.}$$ where the integral of the vertical component of velocity is the vertical distance. The work of gravity depends only on the vertical movement of the curver(t).

A horizontal spring exerts a forceF = (−kx, 0, 0) that is proportional to its deformation in the axial orx-direction. The work of this spring on a body moving along the space curves(t) = (x(t),y(t),z(t)), is calculated using its velocity,v = (v_x,v_y,v_z), to obtain$${\displaystyle W={\int }_0^t\mathbf{F}\cdot \mathbf{v}dt=-{\int }_0^{t}kx{v}_{\text{x}}dt=-{\int }_0^{t}kx\frac{dx}{dt}dt={\int }_{x(t_0)}^{x(t)}kxdx=\frac{1}{2}k{x}^2}$$ For convenience, consider contact with the spring occurs att = 0, then the integral of the product of the distancex and thex-velocity,xv_x, isx²/2.

The function$${\displaystyle U(x)=\frac{1}{2}k{x}^2,}$$ is called the potential energy of a linear spring.

Elastic potential energy is the potential energy of anelastic object (for example abow or a catapult) that is deformed under tension or compression (orstressed in formal terminology). It arises as a consequence of a force that tries to restore the object to its original shape, which is most often theelectromagnetic force between the atoms and molecules that constitute the object. If the stretch is released, the energy is transformed intokinetic energy.

The gravitational potential function, also known asgravitational potential energy, is:$${\displaystyle U=-\frac{GMm}{r},}$$ 

The negative sign follows the convention that work is gained from a loss of potential energy.

The gravitational force between two bodies of massM andm separated by a distancer is given byNewton's law of universal gravitation$${\displaystyle \mathbf{F}=-\frac{GMm}{r^2}\hat{\mathbf{r}},}$$ where${\displaystyle \hat{\mathbf{r}}}$  isa vector of length 1 pointing fromM tom andG is thegravitational constant.

Let the massm move at the velocityv then the work of gravity on this mass as it moves from positionr(t₁) tor(t₂) is given by$${\displaystyle W=-{\int }_{\mathbf{r}(t_1)}^{\mathbf{r}(t_2)}\frac{GMm}{r^3}\mathbf{r}\cdot d\mathbf{r}=-{\int }_{t_1}^{t_2}\frac{GMm}{r^3}\mathbf{r}\cdot \mathbf{v}dt.}$$ The position and velocity of the massm are given by$${\displaystyle \mathbf{r}=r{\mathbf{e}}_r,\mathbf{v}=\dot{r}{\mathbf{e}}_{\text{r}}+r\dot{\theta }{\mathbf{e}}_{\text{t}},}$$ wheree_r ande_t are the radial and tangential unit vectors directed relative to the vector fromM tom. Use this to simplify the formula for work of gravity to,$${\displaystyle W=-{\int }_{t_1}^{t_2}\frac{GmM}{r^3}(r{\mathbf{e}}_{\text{r}})\cdot (\dot{r}{\mathbf{e}}_{\text{r}}+r\dot{\theta }{\mathbf{e}}_{\text{t}})dt=-{\int }_{t_1}^{t_2}\frac{GmM}{r^3}r\dot{r}dt=\frac{GMm}{r(t_2)}-\frac{GMm}{r(t_1)}.}$$ 

This calculation uses the fact that$${\displaystyle \frac{d}{dt}{r}^{-1}=-r^{-2}\dot{r}=-\frac{\dot{r}}{r^2}.}$$ 

The electrostatic force exerted by a chargeQ on another chargeq separated by a distancer is given byCoulomb's law$${\displaystyle \mathbf{F}=\frac{1}{4\pi {\epsilon }_0}\frac{Qq}{r^2}\hat{\mathbf{r}},}$$ where${\displaystyle \hat{\mathbf{r}}}$  is a vector of length 1 pointing fromQ toq andε₀ is thevacuum permittivity.

The workW required to moveq fromA to any pointB in the electrostatic force field is given by the potential function$${\displaystyle U(r)=\frac{1}{4\pi {\epsilon }_0}\frac{Qq}{r}.}$$ 

The potential energy is a function of the state a system is in, and is defined relative to that for a particular state. This reference state is not always a real state; it may also be a limit, such as with the distances between all bodies tending to infinity, provided that the energy involved in tending to that limit is finite, such as in the case ofinverse-square law forces. Any arbitrary reference state could be used; therefore it can be chosen based on convenience.

Typically the potential energy of a system depends on therelative positions of its components only, so the reference state can also be expressed in terms of relative positions.

Gravitational energy is the potential energy associated withgravitational force, as work is required to elevate objects against Earth's gravity. The potential energy due to elevated positions is called gravitational potential energy, and is evidenced by water in an elevated reservoir or kept behind a dam. If an object falls from one point to another point inside a gravitational field, the force of gravity will do positive work on the object, and the gravitational potential energy will decrease by the same amount.

Consider a book placed on top of a table. As the book is raised from the floor to the table, some external force works against the gravitational force. If the book falls back to the floor, the "falling" energy the book receives is provided by the gravitational force. Thus, if the book falls off the table, this potential energy goes to accelerate the mass of the book and is converted intokinetic energy. When the book hits the floor this kinetic energy is converted into heat, deformation, and sound by the impact.

The factors that affect an object's gravitational potential energy are its height relative to some reference point, its mass, and the strength of the gravitational field it is in. Thus, a book lying on a table has less gravitational potential energy than the same book on top of a taller cupboard and less gravitational potential energy than a heavier book lying on the same table. An object at a certain height above the Moon's surface has less gravitational potential energy than at the same height above the Earth's surface because the Moon's gravity is weaker. "Height" in the common sense of the term cannot be used for gravitational potential energy calculations when gravity is not assumed to be a constant. The following sections provide more detail.

The strength of a gravitational field varies with location. However, when the change of distance is small in relation to the distances from the center of the source of the gravitational field, this variation in field strength is negligible and we can assume that the force of gravity on a particular object is constant. Near the surface of the Earth, for example, we assume that the acceleration due to gravity is a constantg = 9.8 m/s² (standard gravity). In this case, a simple expression for gravitational potential energy can be derived using theW =Fd equation forwork, and the equation$${\displaystyle W_{\text{F}}=-\mathrm{\Delta }{U}_{\text{F}}.}$$ 

The amount of gravitational potential energy held by an elevated object is equal to the work done against gravity in lifting it. The work done equals the force required to move it upward multiplied with the vertical distance it is moved (rememberW =Fd). The upward force required while moving at a constant velocity is equal to the weight,mg, of an object, so the work done in lifting it through a heighth is the productmgh. Thus, when accounting only formass,gravity, andaltitude, the equation is:^[8]$${\displaystyle U=mgh}$$ whereU is the potential energy of the object relative to its being on the Earth's surface,m is the mass of the object,g is the acceleration due to gravity, andh is the altitude of the object.^[9]

Hence, the potential difference is$${\displaystyle \mathrm{\Delta }U=mg\mathrm{\Delta }h.}$$ 

However, over large variations in distance, the approximation thatg is constant is no longer valid, and we have to usecalculus and the general mathematical definition of work to determine gravitational potential energy. For the computation of the potential energy, we canintegrate the gravitational force, whose magnitude is given byNewton's law of gravitation, with respect to the distancer between the two bodies. Using that definition, the gravitational potential energy of a system of massesm₁ andM₂ at a distancer using theNewtonian constant of gravitationG is$${\displaystyle U=-G\frac{m_1{M}_2}{r}+K,}$$ whereK is an arbitrary constant dependent on the choice of datum from which potential is measured. Choosing the convention thatK = 0 (i.e. in relation to a point at infinity) makes calculations simpler, albeit at the cost of makingU negative; for why this is physically reasonable, see below.

Given this formula forU, the total potential energy of a system ofn bodies is found by summing, for all$\frac{n(n-1)}{2}$  pairs of two bodies, the potential energy of the system of those two bodies.

Considering the system of bodies as the combined set of small particles the bodies consist of, and applying the previous on the particle level we get the negativegravitational binding energy. This potential energy is more strongly negative than the total potential energy of the system of bodies as such since it also includes the negative gravitational binding energy of each body. The potential energy of the system of bodies as such is the negative of the energy needed to separate the bodies from each other to infinity, while the gravitational binding energy is the energy needed to separate all particles from each other to infinity.$${\displaystyle U=-m\left(G\frac{M_1}{r_1}+G\frac{M_2}{r_2}\right)}$$ therefore,$${\displaystyle U=-m\sum G\frac{M}{r},}$$ 

As with all potential energies, only differences in gravitational potential energy matter for most physical purposes, and the choice of zero point is arbitrary. Given that there is no reasonable criterion for preferring one particular finiter over another, there seem to be only two reasonable choices for the distance at whichU becomes zero:${\displaystyle r=0}$  and${\displaystyle r=\mathrm{\infty }}$ . The choice of${\displaystyle U=0}$  at infinity may seem peculiar, and the consequence that gravitational energy is always negative may seem counterintuitive, but this choice allows gravitational potential energy values to be finite, albeit negative.

Thesingularity at${\displaystyle r=0}$  in the formula for gravitational potential energy means that the only other apparently reasonable alternative choice of convention, with${\displaystyle U=0}$  for⁠${\displaystyle r=0}$ ⁠, would result in potential energy being positive, but infinitely large for all nonzero values ofr, and would make calculations involving sums or differences of potential energies beyond what is possible with thereal number system. Since physicists abhor infinities in their calculations, andr is always non-zero in practice, the choice of${\displaystyle U=0}$  at infinity is by far the more preferable choice, even if the idea of negative energy in agravity well appears to be peculiar at first.

The negative value for gravitational energy also has deeper implications that make it seem more reasonable in cosmological calculations where the total energy of the universe can meaningfully be considered; seeinflation theory for more on this.^[10]

Gravitational potential energy has a number of practical uses, notably the generation ofpumped-storage hydroelectricity. For example, inDinorwig, Wales, there are two lakes, one at a higher elevation than the other. At times when surplus electricity is not required (and so is comparatively cheap), water is pumped up to the higher lake, thus converting the electrical energy (running the pump) to gravitational potential energy. At times of peak demand for electricity, the water flows back down through electrical generator turbines, converting the potential energy into kinetic energy and then back into electricity. The process is not completely efficient and some of the original energy from the surplus electricity is in fact lost to friction.^{[11][12][13][14][15]}

Gravitational potential energy is also used to power clocks in which falling weights operate the mechanism.

It is also used bycounterweights for lifting up anelevator, crane, orsash window.

Roller coasters are an entertaining way to utilize potential energy – chains are used to move a car up an incline (building up gravitational potential energy), to then have that energy converted into kinetic energy as it falls.

Another practical use is utilizing gravitational potential energy to descend (perhaps coast) downhill in transportation such as the descent of an automobile, truck, railroad train, bicycle, airplane, or fluid in a pipeline. In some cases thekinetic energy obtained from the potential energy of descent may be used to start ascending the next grade such as what happens when a road is undulating and has frequent dips. The commercialization of stored energy (in the form of rail cars raised to higher elevations) that is then converted to electrical energy when needed by an electrical grid, is being undertaken in the United States in a system calledAdvanced Rail Energy Storage (ARES).^[16][17][18]

Chemical potential energy is a form of potential energy related to the structural arrangement of atoms or molecules. This arrangement may be the result ofchemical bonds within a molecule or otherwise. Chemical energy of a chemical substance can be transformed to other forms of energy by achemical reaction. As an example, when a fuel is burned the chemical energy is converted to heat, same is the case with digestion of food metabolized in a biological organism. Green plants transformsolar energy to chemical energy through the process known asphotosynthesis, and electrical energy can be converted to chemical energy throughelectrochemical reactions.

The similar termchemical potential is used to indicate the potential of a substance to undergo a change of configuration, be it in the form of a chemical reaction, spatial transport, particle exchange with a reservoir, etc.

An object can have potential energy by virtue of itselectric charge and several forces related to their presence. There are two main types of this kind of potential energy: electrostatic potential energy, electrodynamic potential energy (also sometimes called magnetic potential energy).

Electrostatic potential energy between two bodies in space is obtained from the force exerted by a chargeQ on another chargeq, which is given by$${\displaystyle {\mathbf{F}}_e=-\frac{1}{4\pi {\epsilon }_0}\frac{Qq}{r^2}\hat{\mathbf{r}},}$$ where${\displaystyle \hat{\mathbf{r}}}$  is a vector of length 1 pointing fromQ toq andε₀ is thevacuum permittivity.

If the electric charge of an object can be assumed to be at rest, then it has potential energy due to its position relative to other charged objects. Theelectrostatic potential energy is the energy of an electrically charged particle (at rest) in an electric field. It is defined as thework that must be done to move it from an infinite distance away to its present location, adjusted for non-electrical forces on the object. This energy will generally be non-zero if there is another electrically charged object nearby.

The workW required to moveq fromA to any pointB in the electrostatic force field is given by$${\displaystyle \mathrm{\Delta }{U}_{AB}(\mathbf{r})=-{\int }_A^B{\mathbf{F}}_{\mathbf{e}}\cdot d\mathbf{r}}$$ typically given in J for Joules. A related quantity calledelectric potential (commonly denoted with aV for voltage) is equal to the electric potential energy per unit charge.

The energy of amagnetic moment${\displaystyle \mathit{\mu }}$  in an externally producedmagnetic B-fieldB has potential energy^[19]$${\displaystyle U=-\mathit{\mu }\cdot \mathbf{B}.}$$ 

ThemagnetizationM in a field is$${\displaystyle U=-\frac{1}{2}\int \mathbf{M}\cdot \mathbf{B}dV,}$$ where the integral can be over all space or, equivalently, whereM is nonzero.^[20]Magnetic potential energy is the form of energy related not only to the distance between magnetic materials, but also to the orientation, or alignment, of those materials within the field. For example, the needle of a compass has the lowest magnetic potential energy when it is aligned with the north and south poles of the Earth's magnetic field. If the needle is moved by an outside force, torque is exerted on the magnetic dipole of the needle by the Earth's magnetic field, causing it to move back into alignment. The magnetic potential energy of the needle is highest when its field is in the same direction as the Earth's magnetic field. Two magnets will have potential energy in relation to each other and the distance between them, but this also depends on their orientation. If the opposite poles are held apart, the potential energy will be higher the further they are apart and lower the closer they are. Conversely, like poles will have the highest potential energy when forced together, and the lowest when they spring apart.^[21][22]

Nuclear potential energy is the potential energy of theparticles inside anatomic nucleus. The nuclear particles are bound together by thestrong nuclear force. Their rest mass provides the potential energy for certain kinds of radioactive decay, such asbeta decay.

Nuclear particles like protons and neutrons are not destroyed in fission and fusion processes, but collections of them can have less mass than if they were individually free, in which case this mass difference can be liberated as heat and radiation in nuclear reactions. The process of hydrogen fusion occurring in theSun is an example of this form ofenergy release – 600 million tonnes of hydrogen nuclei are fused into helium nuclei, with a loss of about 4 million tonnes of mass per second. This energy, now in the form ofkinetic energy andgamma rays, keeps the solar core hot even aselectromagnetic radiation carrieselectromagnetic energy into space.

Potential energy is closely linked withforces. If the work done by a force on a body that moves fromA toB does not depend on the path between these points, then the work of this force measured fromA assigns a scalar value to every other point in space and defines ascalar potential field. In this case, the force can be defined as the negative of thevector gradient of the potential field.

For example, gravity is aconservative force. The associated potential is thegravitational potential, often denoted by${\displaystyle \varphi }$  or${\displaystyle V}$ , corresponding to the energy per unit mass as a function of position. The gravitational potential energy of two particles of massM andm separated by a distancer is$${\displaystyle U=-\frac{GMm}{r}.}$$ The gravitational potential (specific energy) of the two bodies is$${\displaystyle \varphi =-\left(\frac{GM}{r}+\frac{Gm}{r}\right)=-\frac{G(M+m)}{r}=-\frac{GMm}{\mu r}=\frac{U}{\mu }}$$ where${\displaystyle \mu }$  is thereduced mass.

The work done against gravity by moving aninfinitesimal mass from point A with${\displaystyle U=a}$  to point B with${\displaystyle U=b}$  is${\displaystyle (b-a)}$  and the work done going back the other way is${\displaystyle (a-b)}$  so that the total work done in moving from A to B and returning to A is$${\displaystyle U_{A\to B\to A}=(b-a)+(a-b)=0.}$$ If the potential is redefined at A to be${\displaystyle a+c}$  and the potential at B to be${\displaystyle b+c}$ , where${\displaystyle c}$  is a constant (i.e.${\displaystyle c}$  can be any number, positive or negative, but it must be the same at A as it is at B) then the work done going from A to B is$${\displaystyle U_{A\to B}=(b+c)-(a+c)=b-a}$$ as before.

In practical terms, this means that one can set the zero of${\displaystyle U}$  and${\displaystyle \varphi }$  anywhere one likes. One may set it to be zero at the surface of theEarth, or may find it more convenient to set zero at infinity (as in the expressions given earlier in this section).

A conservative force can be expressed in the language ofdifferential geometry as aclosed form. AsEuclidean space iscontractible, itsde Rham cohomology vanishes, so every closed form is also anexact form, and can be expressed as the gradient of a scalar field. This gives a mathematical justification of the fact that all conservative forces are gradients of a potential field.

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• Tipler, Paul (2004).Physics for Scientists and Engineers: Mechanics, Oscillations and Waves, Thermodynamics (5th ed.). W. H. Freeman.ISBN 0-7167-0809-4.

• What is potential energy?