Post-Minkowskian expansion

Post-minkowskian vs Post-newtonian expansions

In physics, precisely in the general theory of relativity, post-Minkowskian expansions (PM) or post-Minkowskian approximations are mathematical methods used to find approximate solutions of Einstein's equations by means of a power series development of the metric tensor.

Unlike post-Newtonian expansions (PN), in which the series development is based on a combination of powers of the velocity (which must be negligible compared to that of light) and the gravitational constant, in the post-Minkowskian case the developments are based only on the gravitational constant, allowing analysis even at velocities close to that of light (relativistic). ^[1]

	0PN		1PN		2PN		3PN		4PN		5PN		6PN		7PN
1PM	( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	${\displaystyle v^{6}}$	+	${\displaystyle v^{8}}$	+	${\displaystyle v^{10}}$	+	${\displaystyle v^{12}}$	+	${\displaystyle v^{14}}$	+	...)	${\displaystyle G^{1}}$
2PM			( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	${\displaystyle v^{6}}$	+	${\displaystyle v^{8}}$	+	${\displaystyle v^{10}}$	+	${\displaystyle v^{12}}$	+	...)	${\displaystyle G^{2}}$
3PM					( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	${\displaystyle v^{6}}$	+	${\displaystyle v^{8}}$	+	${\displaystyle v^{10}}$	+	...)	${\displaystyle G^{3}}$
4PM							( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	${\displaystyle v^{6}}$	+	${\displaystyle v^{8}}$	+	...)	${\displaystyle G^{4}}$
5PM									( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	${\displaystyle v^{6}}$	+	...)	${\displaystyle G^{5}}$
6PM											( 1	+	${\displaystyle v^{2}}$	+	${\displaystyle v^{4}}$	+	...)	${\displaystyle G^{6}}$
Comparison table of powers used for PN and PM approximations in the case of two non-rotating bodies. 0PN corresponds to the case of Newton's theory of gravitation. 0PM (not shown) corresponds to the Minkowski flat space. [2]

One of the earliest works on this method of resolution is that of Bruno Bertotti, published in Nuovo Cimento in 1956. ^[3]

See also

• Physics portal

• Effective one-body formalism

References

1. Damour, Thibault (2016-11-07). "Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory". Physical Review D. 94 (10) 104015. arXiv: 1609.00354 . Bibcode:2016PhRvD..94j4015D. doi:10.1103/PhysRevD.94.104015. ISSN   2470-0010. S2CID   106399287.
2. Bern, Zvi; Cheung, Clifford; Roiban, Radu; Shen, Chia-Hsien; Solon, Mikhail P.; Zeng, Mao (2019-08-05). "Black Hole Binary Dynamics from the Double Copy and Effective Theory". Journal of High Energy Physics. 2019 (10): 206. arXiv: 1908.01493 . Bibcode:2019JHEP...10..206B. doi:10.1007/JHEP10(2019)206. ISSN   1029-8479. S2CID   199442337.
3. Bertotti, B. (1956-10-01). "On gravitational motion". Il Nuovo Cimento. 4 (4): 898–906. Bibcode:1956NCim....4..898B. doi:10.1007/BF02746175. ISSN   1827-6121. S2CID   120443098.