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Gravitational waves and energy momentum quanta

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSNConference contribution/Paperpeer-review

Published

Standard

Gravitational waves and energy momentum quanta. / Dereli, Tekin; Tucker, Robin.
Quantum gravity: mathematical models and experimental bounds. ed. / Bertfried Fauser; Jürgen Tolksdorf; Eberhard Zeidler. Basel: Birkhäuser Verlag, 2007. p. 283-292.

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSNConference contribution/Paperpeer-review

Harvard

Dereli, T & Tucker, R 2007, Gravitational waves and energy momentum quanta. in B Fauser, J Tolksdorf & E Zeidler (eds), Quantum gravity: mathematical models and experimental bounds. Birkhäuser Verlag, Basel, pp. 283-292. https://doi.org/10.1007/978-3-7643-7978-0_14

APA

Dereli, T., & Tucker, R. (2007). Gravitational waves and energy momentum quanta. In B. Fauser, J. Tolksdorf, & E. Zeidler (Eds.), Quantum gravity: mathematical models and experimental bounds (pp. 283-292). Birkhäuser Verlag. https://doi.org/10.1007/978-3-7643-7978-0_14

Vancouver

Dereli T, Tucker R. Gravitational waves and energy momentum quanta. In Fauser B, Tolksdorf J, Zeidler E, editors, Quantum gravity: mathematical models and experimental bounds. Basel: Birkhäuser Verlag. 2007. p. 283-292 doi: 10.1007/978-3-7643-7978-0_14

Author

Dereli, Tekin ; Tucker, Robin. / Gravitational waves and energy momentum quanta. Quantum gravity: mathematical models and experimental bounds. editor / Bertfried Fauser ; Jürgen Tolksdorf ; Eberhard Zeidler. Basel : Birkhäuser Verlag, 2007. pp. 283-292

Bibtex

@inproceedings{7f960c4600dd41f49bc05539bebcdda8,
title = "Gravitational waves and energy momentum quanta",
abstract = "We review the role of the classical stress-energy tensor in defining the concept of energy and its conservation in classical field theory. Conserved electromagnetic currents associated with spacetime Killing symmetries are discussed in an attempt to draw analogies with the concepts of photons and gravitons. By embedding Einstein{\textquoteright}s original formulation of General Relativity into a broader context we show that a dynamic covariant description of gravitational stress-energy emerges naturally from a variational principle. A tensor T G is constructed from a contraction of the Bel tensor with a symmetric covariant second degree tensor field Φ that has a form analogous to the stress-energy tensor of the Maxwell field in an arbitrary space-time. For plane-fronted gravitational waves helicity-2 polarised (graviton) states can be identified carrying non-zero energy and momentum.",
author = "Tekin Dereli and Robin Tucker",
year = "2007",
doi = "10.1007/978-3-7643-7978-0_14",
language = "English",
isbn = "9783764379773",
pages = "283--292",
editor = "Bertfried Fauser and J{\"u}rgen Tolksdorf and Eberhard Zeidler",
booktitle = "Quantum gravity",
publisher = "Birkh{\"a}user Verlag",

}

RIS

TY - GEN

T1 - Gravitational waves and energy momentum quanta

AU - Dereli, Tekin

AU - Tucker, Robin

PY - 2007

Y1 - 2007

N2 - We review the role of the classical stress-energy tensor in defining the concept of energy and its conservation in classical field theory. Conserved electromagnetic currents associated with spacetime Killing symmetries are discussed in an attempt to draw analogies with the concepts of photons and gravitons. By embedding Einstein’s original formulation of General Relativity into a broader context we show that a dynamic covariant description of gravitational stress-energy emerges naturally from a variational principle. A tensor T G is constructed from a contraction of the Bel tensor with a symmetric covariant second degree tensor field Φ that has a form analogous to the stress-energy tensor of the Maxwell field in an arbitrary space-time. For plane-fronted gravitational waves helicity-2 polarised (graviton) states can be identified carrying non-zero energy and momentum.

AB - We review the role of the classical stress-energy tensor in defining the concept of energy and its conservation in classical field theory. Conserved electromagnetic currents associated with spacetime Killing symmetries are discussed in an attempt to draw analogies with the concepts of photons and gravitons. By embedding Einstein’s original formulation of General Relativity into a broader context we show that a dynamic covariant description of gravitational stress-energy emerges naturally from a variational principle. A tensor T G is constructed from a contraction of the Bel tensor with a symmetric covariant second degree tensor field Φ that has a form analogous to the stress-energy tensor of the Maxwell field in an arbitrary space-time. For plane-fronted gravitational waves helicity-2 polarised (graviton) states can be identified carrying non-zero energy and momentum.

U2 - 10.1007/978-3-7643-7978-0_14

DO - 10.1007/978-3-7643-7978-0_14

M3 - Conference contribution/Paper

SN - 9783764379773

SP - 283

EP - 292

BT - Quantum gravity

A2 - Fauser, Bertfried

A2 - Tolksdorf, Jürgen

A2 - Zeidler, Eberhard

PB - Birkhäuser Verlag

CY - Basel

ER -