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{{Short description|Type of quantum field}}
{{Unreferenced|date=February 2007}}
In [[quantum field theory]], '''bosonic fields''' are [[quantum field]]s whose quanta are [[boson]]s; that is, they obey [[Bose-Einstein statistics]].
In [[quantum field theory]], a '''bosonic field''' is a [[quantum field]] whose quanta are [[boson]]s; that is, they obey [[Bose–Einstein statistics]]. Bosonic fields obey [[canonical commutation relation]]s, as distinct from the [[canonical anticommutation relation]]s obeyed by [[fermionic fields]].

Examples include [[Scalar field theory#Quantum scalar field theory|scalar fields]], describing spin-0 particles such as the [[Higgs boson]], and gauge fields, describing spin-1 particles such as the [[photon]].

==Basic properties==

Free (non-interacting) bosonic fields obey canonical commutation relations. Those relations also hold for interacting bosonic fields in the interaction picture, where the fields evolve in time as if free and the effects of the interaction are encoded in the evolution of the states. It is these commutation relations that imply Bose–Einstein statistics for the field quanta.


==Examples==
==Examples==
Examples of bosonic fields include [[scalar field (physics)|scalar field]]s, [[vector field (physics)|vector field]]s, and [[tensor field]]s, as characterized by their properties under [[Lorentz transformation]]s (or equivalently by their spin, 0, 1 and 2, respectively). Physical examples, in the same order, are: the Higgs field, the photon field and the graviton field. While the first one remains to be observed, it is widely believed to exist. Of the last two, only the photon field can be quantized using the conventional methods of canonical or path integral quantization. This has led to the theory of quantum electrodynamics, arguably the most successful theory in Physics. Quantization of gravity, on the other hand, is a long standing problem that has led to theories such as [[string theory]].
Examples of bosonic fields include [[scalar field (physics)|scalar field]]s, [[gauge field]]s, and [[symmetric tensor|symmetric 2-tensor]] [[tensor field|fields]], which are characterized by their [[covariance]] under [[Lorentz transformation]]s and have spins 0, 1 and 2, respectively. Physical examples, in the same order, are the Higgs field, the photon field, and the graviton field. Of the last two, only the photon field can be quantized using the conventional methods of canonical or path integral quantization. This has led to the theory of [[quantum electrodynamics]], one of the most successful theories in physics. [[Quantum gravity|Quantization of gravity]], on the other hand, is a long-standing problem that has led to development of theories such as [[string theory]] and [[loop quantum gravity]].


==Spin and statistics==
==Properties==
By definition, free (non-interacting) bosonic fields obey [[canonical commutation relation]]s. Those relations also hold for interacting bosonic fields in the interaction picture, where the fields evolve in time as if free and the effects of the interaction are encoded in the evolution of the states. It is these commutation relations that imply Bose-Einstein statistics for the field quanta.


As implied by the [[Spin-statistics theorem]], quantization of local, relativistic field theories in 3+1 dimensions may lead to either bosonic or fermionic quantum fields, i.e., fields obeying commutation or anti-commutation relations, according to whether they have integral or half integral spin, respectively. In this sense, bosonic fields are one of the two theoretically possible types of quantum field, namely those with integral spin. In lower dimensions, e.g. 2+1, one may have other types of fields, such as [[anyon]]s, that obey [[fractional statistics]].
The [[spin–statistics theorem]] implies that quantization of local, relativistic field theories in 3+1 dimensions may lead either to bosonic or fermionic quantum fields, i.e., fields obeying commutation or anti-commutation relations, according to whether they have [[integer]] or [[half-integer]] spin, respectively. Thus bosonic fields are one of the two theoretically possible types of quantum field, namely those corresponding to particles with integer spin.


In non-relativistic many-body theory, the spin and the statistical properties of the quanta are not directly related. In fact, the commutation or anti-commutation relations are assumed
In a non-relativistic many-body theory, the spin and the statistical properties of the quanta are not directly related. In fact, the commutation or anti-commutation relations are assumed based on whether the theory one intends to study corresponds to particles obeying Bose–Einstein or Fermi–Dirac statistics. In this context the spin remains an internal quantum number that is only phenomenologically related to the statistical properties of the quanta. Examples of non-relativistic bosonic fields include those describing cold bosonic atoms, such as Helium-4.

based on whether the theory one intends to study corresponds to particles obeying Bose-Einstein or Fermi-Dirac statistics. In this context the spin remains an internal quantum number that is only phenomenologically related to the statistical properties of the quanta.
It must be stressed that such non-relativistic fields arise merely as an extremely convenient 're-packaging' of the many-body wave function describing the state of the system. This is to be contrasted with their relativistic counterparts (described above): they are a necessary consequence of the consistent union of relativity and quantum mechanics.
Such non-relativistic fields are not as fundamental as their relativistic counterparts: they provide a convenient 're-packaging' of the many-body wave function describing the state of the system, whereas the relativistic fields described above are a necessary consequence of the consistent union of relativity and quantum mechanics.
Examples of non-relativistic bosonic fields include those describing cold bosonic atoms, such as Helium-4.


==See also==
==See also==
*[[Fermionic field]]
*[[Quantum triviality]]
*[[Spin-statistics theorem]]
*[[Composite field]]
*[[Auxiliary field]]

==References==
* {{cite journal | last=Edwards | first=David A. | title=Mathematical foundations of quantum field theory: Fermions, gauge fields, and supersymmetry part I: Lattice field theories | journal=International Journal of Theoretical Physics | publisher=Springer Nature | volume=20 | issue=7 | year=1981 | issn=0020-7748 | doi=10.1007/bf00669437 | pages=503–517| bibcode=1981IJTP...20..503E | s2cid=120108219 }}
* {{cite journal | last1=Hoffmann | first1=Scott E. | last2=Corney | first2=Joel F. | last3=Drummond | first3=Peter D. | title=Hybrid phase-space simulation method for interacting Bose fields | journal=Physical Review A | publisher=American Physical Society (APS) | volume=78 | issue=1 | date=18 July 2008 | issn=1050-2947 | doi=10.1103/physreva.78.013622 | page=013622| arxiv=0803.1887 | bibcode=2008PhRvA..78a3622H | s2cid=17652144 }}
* Peskin, M and Schroeder, D. (1995). ''An Introduction to Quantum Field Theory'', Westview Press.
* Srednicki, Mark (2007). ''[http://www.physics.ucsb.edu/~mark/qft.html Quantum Field Theory] {{Webarchive|url=https://web.archive.org/web/20110725093208/http://www.physics.ucsb.edu/~mark/qft.html |date=2011-07-25 }}'', Cambridge University Press, {{ISBN|978-0-521-86449-7}}.
* Weinberg, Steven (1995). ''The Quantum Theory of Fields'', (3 volumes) Cambridge University Press.


[[Category:Quantum field theory]]
[[Category:Quantum field theory]]

Latest revision as of 04:02, 21 October 2023

In quantum field theory, a bosonic field is a quantum field whose quanta are bosons; that is, they obey Bose–Einstein statistics. Bosonic fields obey canonical commutation relations, as distinct from the canonical anticommutation relations obeyed by fermionic fields.

Examples include scalar fields, describing spin-0 particles such as the Higgs boson, and gauge fields, describing spin-1 particles such as the photon.

Basic properties

[edit]

Free (non-interacting) bosonic fields obey canonical commutation relations. Those relations also hold for interacting bosonic fields in the interaction picture, where the fields evolve in time as if free and the effects of the interaction are encoded in the evolution of the states. It is these commutation relations that imply Bose–Einstein statistics for the field quanta.

Examples

[edit]

Examples of bosonic fields include scalar fields, gauge fields, and symmetric 2-tensor fields, which are characterized by their covariance under Lorentz transformations and have spins 0, 1 and 2, respectively. Physical examples, in the same order, are the Higgs field, the photon field, and the graviton field. Of the last two, only the photon field can be quantized using the conventional methods of canonical or path integral quantization. This has led to the theory of quantum electrodynamics, one of the most successful theories in physics. Quantization of gravity, on the other hand, is a long-standing problem that has led to development of theories such as string theory and loop quantum gravity.

Spin and statistics

[edit]

The spin–statistics theorem implies that quantization of local, relativistic field theories in 3+1 dimensions may lead either to bosonic or fermionic quantum fields, i.e., fields obeying commutation or anti-commutation relations, according to whether they have integer or half-integer spin, respectively. Thus bosonic fields are one of the two theoretically possible types of quantum field, namely those corresponding to particles with integer spin.

In a non-relativistic many-body theory, the spin and the statistical properties of the quanta are not directly related. In fact, the commutation or anti-commutation relations are assumed based on whether the theory one intends to study corresponds to particles obeying Bose–Einstein or Fermi–Dirac statistics. In this context the spin remains an internal quantum number that is only phenomenologically related to the statistical properties of the quanta. Examples of non-relativistic bosonic fields include those describing cold bosonic atoms, such as Helium-4.

Such non-relativistic fields are not as fundamental as their relativistic counterparts: they provide a convenient 're-packaging' of the many-body wave function describing the state of the system, whereas the relativistic fields described above are a necessary consequence of the consistent union of relativity and quantum mechanics.

See also

[edit]

References

[edit]
  • Edwards, David A. (1981). "Mathematical foundations of quantum field theory: Fermions, gauge fields, and supersymmetry part I: Lattice field theories". International Journal of Theoretical Physics. 20 (7). Springer Nature: 503–517. Bibcode:1981IJTP...20..503E. doi:10.1007/bf00669437. ISSN 0020-7748. S2CID 120108219.
  • Hoffmann, Scott E.; Corney, Joel F.; Drummond, Peter D. (18 July 2008). "Hybrid phase-space simulation method for interacting Bose fields". Physical Review A. 78 (1). American Physical Society (APS): 013622. arXiv:0803.1887. Bibcode:2008PhRvA..78a3622H. doi:10.1103/physreva.78.013622. ISSN 1050-2947. S2CID 17652144.
  • Peskin, M and Schroeder, D. (1995). An Introduction to Quantum Field Theory, Westview Press.
  • Srednicki, Mark (2007). Quantum Field Theory Archived 2011-07-25 at the Wayback Machine, Cambridge University Press, ISBN 978-0-521-86449-7.
  • Weinberg, Steven (1995). The Quantum Theory of Fields, (3 volumes) Cambridge University Press.