Love number
The Love numbers (h, k, and l) are dimensionless parameters that measure the rigidity of a planetary body and the susceptibility of its shape to change in response to a tidal potential.
In 1909, Augustus Edward Hough Love introduced the values h and k which characterize the overall elastic response of the Earth to the tides ― Earth tides or body tides.[1] Later, in 1912, Toshi Shida added a third Love number, l, which was needed to obtain a complete overall description of the solid Earth's response to the tides.[2]
Definitions
The Love number h is defined as the ratio of the body tide to the height of the static equilibrium tide;[3] also defined as the vertical (radial) displacement or variation of the planet's elastic properties. In terms of the tide generating potential , the displacement is where is latitude, is east longitude and is acceleration due to gravity.[4] For a hypothetical solid Earth . For a liquid Earth, one would expect . However, the deformation of the sphere causes the potential field to change, and thereby deform the sphere even more. The theoretical maximum is . For the real Earth, lies between 0 and 1.
The Love number k is defined as the cubical dilation or the ratio of the additional potential (self-reactive force) produced by the deformation of the deforming potential. It can be represented as , where for a rigid body.[4]
The Love number l represents the ratio of the horizontal (transverse) displacement of an element of mass of the planet's crust to that of the corresponding static ocean tide.[3] In potential notation the transverse displacement is , where is the horizontal gradient operator. As with h and k, for a rigid body.[4]
Values
According to Cartwright, "An elastic solid spheroid will yield to an external tide potential of spherical harmonic degree 2 by a surface tide and the self-attraction of this tide will increase the external potential by ."[5] The magnitudes of the Love numbers depend on the rigidity and mass distribution of the spheroid. Love numbers , , and can also be calculated for higher orders of spherical harmonics.
For elastic Earth the Love numbers lie in the range: , and .[3]
For Earth's tides one can calculate the tilt factor as and the gravimetric factor as , where subscript two is assumed.[5]
Neutron stars are thought to have high rigidity in the crust, and thus a low Love number; ,[6][7] while black holes simply have .[8][9]
References
- Love Augustus Edward Hough. The yielding of the earth to disturbing forces 82 Proc. R. Soc. Lond. A 1909 http://doi.org/10.1098/rspa.1909.0008
- TOSHI SHIDA, On the Body Tides of the Earth, A Proposal for the International Geodetic Association, Proceedings of the Tokyo Mathematico-Physical Society. 2nd Series, 1911-1912, Volume 6, Issue 16, Pages 242-258, ISSN 2185-2693, doi:10.11429/ptmps1907.6.16_242.
- "Tidal Deformation of the Solid Earth: A Finite Difference Discretization", S.K.Poulsen; Niels Bohr Institute, University of Copenhagen; p 24; Archived 2016-10-11 at the Wayback Machine
- Earth Tides; D.C.Agnew, University of California; 2007; 174
- Tides: A Scientific History; David E. Cartwright; Cambridge University Press, 1999, ISBN 0-521-62145-3; pp 140–141,224
- Yazadjiev, Stoytcho S.; Doneva, Daniela D.; Kokkotas, Kostas D. (October 2018). "Tidal Love numbers of neutron stars in f(R) gravity". The European Physical Journal C. 78 (10): 818. doi:10.1140/epjc/s10052-018-6285-z. PMC 6244867. PMID 30524193.
- Hinderer, Tanja; Lackey, Benjamin D.; Lang, Ryan N.; Read, Jocelyn S. (23 June 2010). "Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral". Physical Review D. 81 (12): 123016. doi:10.1103/PhysRevD.81.123016. hdl:1721.1/64461. S2CID 14819350.
- Pani, Paolo; Gualtieri, Leonardo; Maselli, Andrea; Ferrari, Valeria (7 July 2015). "Tidal deformations of a spinning compact object". Physical Review D. 92 (2): 024010. arXiv:1503.07365. doi:10.1103/PhysRevD.92.024010. S2CID 117779102.
- Landry, Philippe; Poisson, Eric (19 May 2015). "Tidal deformation of a slowly rotating material body: External metric". Physical Review D. 91 (10): 104018. arXiv:1503.07366. doi:10.1103/PhysRevD.91.104018. S2CID 118363442.