Charge conservation

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This article is about the conservation of electric charge. For a general theoretical concept, see charge (physics).

In physics, charge conservation is the principle that electric charge can neither be created nor destroyed. The net quantity of electric charge, the amount of positive charge minus the amount of negative charge in the universe, is always conserved. Charge conservation was first proposed by British scientist William Watson in 1746 and American statesman and scientist Benjamin Franklin in 1747, although the first convincing proof was given by Michael Faraday in 1843.[1][2]

it is now discovered and demonstrated, both here and in Europe, that the Electrical Fire is a real Element, or Species of Matter, not created by the Friction, but collected only.

— Benjamin Franklin, Letter to Cadwallader Colden, 5 June 1747[3]

Charge conservation is a physical law that states that the change in the amount of electric charge in any volume of space is exactly equal to the amount of charge flowing into the volume minus the amount of charge flowing out of the volume. In essence, charge conservation is an accounting relationship between the amount of charge in a region and the flow of charge into and out of that region.

Mathematically, we can state the law as a continuity equation:

Q(t) is the quantity of electric charge in a specific volume at time t, QIN is the amount of charge flowing into the volume between time t1 and t2, and QOUT is the amount of charge flowing out of the volume during the same time period.

This does not mean that individual positive and negative charges cannot be created or destroyed. Electric charge is carried by subatomic particles such as electrons and protons, which can be created and destroyed. In particle physics, charge conservation means that in elementary particle reactions that create charged particles, equal numbers of positive and negative particles are always created, keeping the net amount of charge unchanged. Similarly, when particles are destroyed, equal numbers of positive and negative charges are destroyed.

Although conservation of charge requires that the total quantity of charge in the universe is constant, it leaves open the question of what that quantity is. Most evidence indicates that the net charge in the universe is zero;[4][5] that is, there are equal quantities of positive and negative charge.

Formal statement of the law[edit]

In electromagnetic field theory, vector calculus can be used to express the law in terms of charge density ρ (in coulombs per cubic meter) and electric current density J (in amperes per square meter). This is called the charge continuity equation

The term on the left is the rate of change of the charge density ρ at a point. The term on the right is the divergence of the current density J at the same point. The equation equates these two factors, which says that the only way for the charge density at a point to change is for a current of charge to flow into or out of the point. This statement is equivalent to a conservation of four-current.

Mathematical derivation[edit]

The net current into a volume is

where S = ∂V is the boundary of V oriented by outward-pointing normals, and dS is shorthand for NdS, the outward pointing normal of the boundary V. Here J is the current density (charge per unit area per unit time) at the surface of the volume. The vector points in the direction of the current.

From the Divergence theorem this can be written

Charge conservation requires that the net current into a volume must necessarily equal the net change in charge within the volume.

The total charge q in volume V is the integral (sum) of the charge density in V


Equating (1) and (2) gives

Since this is true for every volume, we have in general

Connection to gauge invariance[edit]

Charge conservation can also be understood as a consequence of symmetry through Noether's theorem, a central result in theoretical physics that asserts that each conservation law is associated with a symmetry of the underlying physics. The symmetry that is associated with charge conservation is the global gauge invariance of the electromagnetic field.[6] This is related to the fact that the electric and magnetic fields are not changed by different choices of the value representing the zero point of electrostatic potential . However the full symmetry is more complicated, and also involves the vector potential . The full statement of gauge invariance is that the physics of an electromagnetic field are unchanged when the scalar and vector potential are shifted by the gradient of an arbitrary scalar field :

In quantum mechanics the scalar field is equivalent to a phase shift in the wavefunction of the charged particle:

so gauge invariance is equivalent to the well known fact that changes in the phase of a wavefunction are unobservable, and only changes in the magnitude of the wavefunction result in changes to the probability function . This is the ultimate theoretical origin of charge conservation.

Gauge invariance is a very important, well established property of the electromagnetic field and has many testable consequences. The theoretical justification for charge conservation is greatly strengthened by being linked to this symmetry. For example, local gauge invariance also requires that the photon be massless, so the good experimental evidence that the photon has zero mass is also strong evidence that charge is conserved.[7]

Even if gauge symmetry is exact, however, there might be apparent electric charge non-conservation if charge could leak from our normal 3-dimensional space into hidden extra dimensions.[8][9]

Experimental evidence[edit]

Simple arguments rule out some types of charge nonconservation. For example, the magnitude of the elementary charge on positive and negative particles must be extremely close to equal, differing by no more than a factor of 10−21 for the case of protons and electrons.[10] Ordinary matter contains equal numbers of positive and negative particles, protons and electrons, in enormous quantities. If the elementary charge on the electron and proton were even slightly different, all matter would have a large electric charge and would be mutually repulsive.

The best experimental tests of electric charge conservation are searches for particle decays that would be allowed if electric charge is not always conserved. No such decays have ever been seen.[11] The best experimental test comes from searches for the energetic photon from an electron decaying into a neutrino and a single photon:

  e → ν + γ   mean lifetime is greater than 6.6×1028 years (90% Confidence Level),[12][13]

but there are theoretical arguments that such single-photon decays will never occur even if charge is not conserved.[14] Charge disappearance tests are sensitive to decays without energetic photons, other unusual charge violating processes such as an electron spontaneously changing into a positron,[15] and to electric charge moving into other dimensions. The best experimental bounds on charge disappearance are:

  e → anything mean lifetime is greater than 6.4×1024 years (68% CL)[16]
n → p + ν + ν charge non-conserving decays are less than 8 × 10−27 (68% CL) of all neutron decays[17]

See also[edit]


  1. ^ Heilbron, J.L. (1979). Electricity in the 17th and 18th centuries: a study of early Modern physics. University of California Press. p. 330. ISBN 0-520-03478-3. 
  2. ^ Purrington, Robert D. (1997). Physics in the Nineteenth Century. Rutgers University Press. p. 33. ISBN 0813524423. 
  3. ^ The Papers of Benjamin Franklin. 3. Yale University Press. 1961. p. 142. 
  4. ^ S. Orito; M. Yoshimura (1985). "Can the Universe be Charged?". Physical Review Letters. 54 (22): 2457–2460. Bibcode:1985PhRvL..54.2457O. doi:10.1103/PhysRevLett.54.2457. 
  5. ^ E. Masso; F. Rota (2002). "Primordial helium production in a charged universe". Physics Letters B. 545 (3–4): 221–225. arXiv:astro-ph/0201248Freely accessible. Bibcode:2002PhLB..545..221M. doi:10.1016/S0370-2693(02)02636-9. 
  6. ^ Bettini, Alessandro (2008). Introduction to Elementary Particle Physics. UK: Cambridge University Press. pp. 164–165. ISBN 0-521-88021-1. 
  7. ^ A.S. Goldhaber; M.M. Nieto (2010). "Photon and Graviton Mass Limits". Reviews of Modern Physics. 82 (1): 939–979. arXiv:0809.1003Freely accessible. Bibcode:2010RvMP...82..939G. doi:10.1103/RevModPhys.82.939. ; see Section II.C Conservation of Electric Charge
  8. ^ S.Y. Chu (1996). "Gauge-Invariant Charge Nonconserving Processes and the Solar Neutrino Puzzle". Modern Physics Letters A. 11 (28): 2251–2257. Bibcode:1996MPLA...11.2251C. doi:10.1142/S0217732396002241. 
  9. ^ S.L. Dubovsky; V.A. Rubakov; P.G. Tinyakov (2000). "Is the electric charge conserved in brane world?". Journal of High Energy Physics. August (8): 315–318. arXiv:hep-ph/0007179Freely accessible. Bibcode:1979PhLB...84..315I. doi:10.1016/0370-2693(79)90048-0. 
  10. ^ Patrignani, C. et al (Particle Data Group) (2016). "The Review of Particle Physics" (PDF). Chinese Physics C. IOP Publishing. 40 (100001). Retrieved March 26, 2017. 
  11. ^ Particle Data Group (May 2010). "Tests of Conservation Laws" (PDF). Journal of Physics G. 37 (7A): 89–98. Bibcode:2010JPhG...37g5021N. doi:10.1088/0954-3899/37/7A/075021. 
  12. ^ Agostini, M.; et al. (Borexino Coll.) (2015). "Test of Electric Charge Conservation with Borexino". Physical Review Letters. 115 (23): 231802. arXiv:1509.01223Freely accessible. Bibcode:2015PhRvL.115w1802A. doi:10.1103/PhysRevLett.115.231802. PMID 26684111. 
  13. ^ Back, H.O.; et al. (Borexino Coll.) (2002). "Search for electron decay mode e → γ + ν with prototype of Borexino detector". Physics Letters B. 525 (1–2): 29–40. Bibcode:2002PhLB..525...29B. doi:10.1016/S0370-2693(01)01440-X. 
  14. ^ L.B. Okun (1989). "Comments on Testing Charge Conservation and Pauli Exclusion Principle". Comments on Nuclear and Particle Physics. 19 (3): 99–116. 
  15. ^ R.N. Mohapatra (1987). "Possible Nonconservation of Electric Charge". Physical Review Letters. 59 (14): 1510–1512. Bibcode:1987PhRvL..59.1510M. doi:10.1103/PhysRevLett.59.1510. PMID 10035254. 
  16. ^ P. Belli; et al. (1999). "Charge non-conservation restrictions from the nuclear levels excitation of 129Xe induced by the electron's decay on the atomic shell". Physics Letters B. 465 (1–4): 315–322. Bibcode:1999PhLB..465..315B. doi:10.1016/S0370-2693(99)01091-6.  This is the most stringent of several limits given in Table 1 of this paper.
  17. ^ Norman, E.B.; Bahcall, J.N.; Goldhaber, M. (1996). "Improved limit on charge conservation derived from 71Ga solar neutrino experiments". Physical Review. D53 (7): 4086–4088. Bibcode:1996PhRvD..53.4086N. doi:10.1103/PhysRevD.53.4086. 

Further reading[edit]