A bound state is a composite of two or more fundamental building blocks, such as particles, atoms, or bodies, that behaves as a single object and in which energy is required to split them.^{[1]}
In quantum physics, a bound state is a quantum state of a particle subject to a potential such that the particle has a tendency to remain localized in one or more regions of space.^{[2]} The potential may be external or it may be the result of the presence of another particle; in the latter case, one can equivalently define a bound state as a state representing two or more particles whose interaction energy exceeds the total energy of each separate particle. One consequence is that, given a potential vanishing at infinity, negativeenergy states must be bound. The energy spectrum of the set of bound states are most commonly discrete, unlike scattering states of free particles, which have a continuous spectrum.
Although not bound states in the strict sense, metastable states with a net positive interaction energy, but long decay time, are often considered unstable bound states as well and are called "quasibound states".^{[3]} Examples include radionuclides and Rydberg atoms.^{[4]}
In relativistic quantum field theory, a stable bound state of n particles with masses corresponds to a pole in the Smatrix with a centerofmass energy less than . An unstable bound state shows up as a pole with a complex centerofmass energy.
Examples
 A proton and an electron can move separately; when they do, the total centerofmass energy is positive, and such a pair of particles can be described as an ionized atom. Once the electron starts to "orbit" the proton, the energy becomes negative, and a bound state – namely the hydrogen atom – is formed. Only the lowestenergy bound state, the ground state, is stable. Other excited states are unstable and will decay into stable (but not other unstable) bound states with less energy by emitting a photon.
 A positronium "atom" is an unstable bound state of an electron and a positron. It decays into photons.
 Any state in the quantum harmonic oscillator is bound, but has positive energy. Note that , so the below does not apply.
 A nucleus is a bound state of protons and neutrons (nucleons).
 The proton itself is a bound state of three quarks (two up and one down; one red, one green and one blue). However, unlike the case of the hydrogen atom, the individual quarks can never be isolated. See confinement.
 The Hubbard and Jaynes–Cummings–Hubbard (JCH) models support similar bound states. In the Hubbard model, two repulsive bosonic atoms can form a bound pair in an optical lattice.^{[5]}^{[6]}^{[7]} The JCH Hamiltonian also supports twopolariton bound states when the photonatom interaction is sufficiently strong.^{[8]}
Definition
Let σfinite measure space be a probability space associated with separable complex Hilbert space . Define a oneparameter group of unitary operators , a density operator and an observable on . Let be the induced probability distribution of with respect to . Then the evolution
is bound with respect to if
 ,
where .^{[dubious – discuss]}^{[9]}
A quantum particle is in a bound state if at no point in time it is found “too far away" from any finite region . Using a wave function representation, for example, this means
such that
In general, a quantum state is a bound state if and only if it is finitely normalizable for all times .^{[10]} Furthermore, a bound state lies within the pure point part of the spectrum of if and only if it is an eigenstate of .^{[11]}
More informally, "boundedness" results foremost from the choice of domain of definition and characteristics of the state rather than the observable.^{[nb 1]} For a concrete example: let and let be the position operator. Given compactly supported and .
 If the state evolution of "moves this wave package to the right", e.g. if for all , then is not bound state with respect to position.
 If does not change in time, i.e. for all , then is bound with respect to position.
 More generally: If the state evolution of "just moves inside a bounded domain", then is bound with respect to position.
Properties
As finitely normalizable states must lie within the pure point part of the spectrum, bound states must lie within the pure point part. However, as Neumann and Wigner pointed out, it is possible for the energy of a bound state to be located in the continuous part of the spectrum. This phenomenon is referred to as bound state in the continuum.^{[12]}^{[13]}
Positionbound states
Consider the oneparticle Schrödinger equation. If a state has energy , then the wavefunction ψ satisfies, for some
so that ψ is exponentially suppressed at large x. This behaviour is wellstudied for smoothly varying potentials in the WKB approximation for wavefunction, where an oscillatory behaviour is observed if the right hand side of the equation is negative and growing/decaying behaviour if it is positive.^{[14]} Hence, negative energystates are bound if V vanishes at infinity.
NonDegeneracy in One dimensional bound states
1D bound states can be shown to be non degenerate in energy for wellbehaved wavefunctions that decay to zero at infinities. This need not hold true for wavefunction in higher dimensions. Due to the property of nondegenerate states, one dimensional bound states can always be expressed as real wavefunctions.
Proof 

Consider two energy eigenstates states and with same energy eigenvalue. Then since, the Schrodinger equation, which is expressed as: is satisfied for i = 1 and 2, subtracting the two equations gives: which can be rearranged to give the condition: Since , taking limit of x going to infinity on both sides, the wavefunctions vanish and gives .
Furthermore it can be shown that these wavefunctions can always be represented by a completely real wavefunction. Define real functions and such that . Then, from Schrodinger's equation: we get that, since the terms in the equation are all real values: applies for i = 1 and 2. Thus every 1D bound state can be represented by completely real eigenfunctions. Note that real function representation of wavefunctions from this proof applies for all nondegenerate states in general.

Node theorem
Node theorem states that nth bound wavefunction ordered according to increasing energy has exactly n1 nodes, ie. points where . Due to the form of Schrödinger's time independent equations, it is not possible for a physical wavefunction to have since it corresponds to solution.^{[15]}
Requirements
A boson with mass m_{χ} mediating a weakly coupled interaction produces an Yukawalike interaction potential,
 ,
where , g is the gauge coupling constant, and ƛ_{i} = ℏ/m_{i}c is the reduced Compton wavelength. A scalar boson produces a universally attractive potential, whereas a vector attracts particles to antiparticles but repels like pairs. For two particles of mass m_{1} and m_{2}, the Bohr radius of the system becomes
and yields the dimensionless number
 .
In order for the first bound state to exist at all, . Because the photon is massless, D is infinite for electromagnetism. For the weak interaction, the Z boson's mass is 91.1876±0.0021 GeV/c^{2}, which prevents the formation of bound states between most particles, as it is 97.2 times the proton's mass and 178,000 times the electron's mass.
Note however that if the Higgs interaction didn't break electroweak symmetry at the electroweak scale, then the SU(2) weak interaction would become confining.^{[16]}
See also
 Bethe–Salpeter equation
 Bound state in the continuum
 Composite field
 Cooper pair
 Resonance (particle physics)
 Levinson's theorem
Remarks
 ^ See Expectation value (quantum mechanics) for an example.
References
 ^ "Bound state  Oxford Reference".
 ^ Blanchard, Philippe; Brüning, Erwin (2015). Mathematical Methods in Physics. Birkhäuser. p. 430. ISBN 9783319140445.
 ^ Sakurai, Jun (1995). "7.8". In Tuan, San (ed.). Modern Quantum Mechanics (Revised ed.). Reading, Mass: AddisonWesley. pp. 418–9. ISBN 0201539292.
Suppose the barrier were infinitely high ... we expect bound states, with energy E > 0. ... They are stationary states with infinite lifetime. In the more realistic case of a finite barrier, the particle can be trapped inside, but it cannot be trapped forever. Such a trapped state has a finite lifetime due to quantummechanical tunneling. ... Let us call such a state quasibound state because it would be an honest bound state if the barrier were infinitely high.
 ^ Gallagher, Thomas F. (19940915). "Oscillator strengths and lifetimes". Rydberg Atoms (1 ed.). Cambridge University Press. pp. 38–49. doi:10.1017/cbo9780511524530.005. ISBN 9780521385312.
 ^ K. Winkler; G. Thalhammer; F. Lang; R. Grimm; J. H. Denschlag; A. J. Daley; A. Kantian; H. P. Buchler; P. Zoller (2006). "Repulsively bound atom pairs in an optical lattice". Nature. 441 (7095): 853–856. arXiv:condmat/0605196. Bibcode:2006Natur.441..853W. doi:10.1038/nature04918. PMID 16778884. S2CID 2214243.
 ^ Javanainen, Juha; Odong Otim; Sanders, Jerome C. (Apr 2010). "Dimer of two bosons in a onedimensional optical lattice". Phys. Rev. A. 81 (4): 043609. arXiv:1004.5118. Bibcode:2010PhRvA..81d3609J. doi:10.1103/PhysRevA.81.043609. S2CID 55445588.
 ^ M. Valiente & D. Petrosyan (2008). "Twoparticle states in the Hubbard model". J. Phys. B: At. Mol. Opt. Phys. 41 (16): 161002. arXiv:0805.1812. Bibcode:2008JPhB...41p1002V. doi:10.1088/09534075/41/16/161002. S2CID 115168045.
 ^ Max T. C. Wong & C. K. Law (May 2011). "Twopolariton bound states in the JaynesCummingsHubbard model". Phys. Rev. A. 83 (5). American Physical Society: 055802. arXiv:1101.1366. Bibcode:2011PhRvA..83e5802W. doi:10.1103/PhysRevA.83.055802. S2CID 119200554.
 ^ Reed, M.; Simon, B. (1980). Methods of Modern Mathematical Physics: I: Functional analysis. Academic Press. p. 303. ISBN 9780125850506.
 ^ Ruelle, D. (1969). "A remark on bound states in potentialscattering theory" (PDF). Il Nuovo Cimento A. 61 (4). Springer Science and Business Media LLC. doi:10.1007/bf02819607. ISSN 03693546.
 ^ Simon, B. (1978). "An Overview of Rigorous Scattering Theory". p. 3.
 ^ Stillinger, Frank H.; Herrick, David R. (1975). "Bound states in the continuum". Physical Review A. 11 (2). American Physical Society (APS): 446–454. doi:10.1103/physreva.11.446. ISSN 05562791.
 ^ Hsu, Chia Wei; Zhen, Bo; Stone, A. Douglas; Joannopoulos, John D.; Soljačić, Marin (2016). "Bound states in the continuum". Nature Reviews Materials. 1 (9). Springer Science and Business Media LLC. doi:10.1038/natrevmats.2016.48. hdl:1721.1/108400. ISSN 20588437.
 ^ Hall, Brian C. (2013). Quantum theory for mathematicians. Graduate texts in mathematics. New York Heidelberg$fDordrecht London: Springer. p. 316320. ISBN 9781461471158.
 ^ Berezin, F. A. (1991). The Schrödinger equation. Dordrecht ; Boston : Kluwer Academic Publishers. pp. 64–66. ISBN 9780792312185.
 ^ Claudson, M.; Farhi, E.; Jaffe, R. L. (1 August 1986). "Strongly coupled standard model". Physical Review D. 34 (3): 873–887. Bibcode:1986PhRvD..34..873C. doi:10.1103/PhysRevD.34.873. PMID 9957220.
Further reading
 Blanchard, Philippe; Brüning, Edward (2015). "Some Applications of the Spectral Representation". Mathematical Methods in Physics: Distributions, Hilbert Space Operators, Variational Methods, and Applications in Quantum Physics (2nd ed.). Switzerland: Springer International Publishing. p. 431. ISBN 9783319140445.
 Gustafson, Stephen J.; Sigal, Israel Michael (2011). "Spectrum and Dynamics". Mathematical Concepts of Quantum Mechanics (2nd ed.). Berlin, Heidelberg: SpringerVerlag. p. 50. ISBN 9783642218651.
 Ruelle, David (9 January 2016). "A Remark on Bound States in PotentialScattering Theory" (PDF). Nuovo Cimento A. 61 (June 1969): 655–662. doi:10.1007/BF02819607. S2CID 56050354. Retrieved 27 December 2021.