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2016 | OriginalPaper | Chapter

A Closed-Form Solution for a Linear Viscoelastic Self-gravitating Sphere

Authors : Wolfgang H. Müller, Elena N. Vilchevskaya

Published in: Advanced Methods of Continuum Mechanics for Materials and Structures

Publisher: Springer Singapore

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Abstract

Following up on the classical solutions by Love for a linear-elastic self-gravitating sphere, this paper presents the corresponding extension to a linear viscoelastic body of the Kelvin–Voigt type. The solution is expressed in closed form by making use of Laplace transforms. Applications to the genesis of terrestrial planets are sought and the evolution of the Love radius and possible extensions to large deformations are discussed. As a new result, it turns out that in the early days of planet formation there is no Love radius and that it takes time for the Love radius to develop.

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Appendix
Available only for authorised users
Footnotes
1
It is said that also the gas giants initially need a rocky core of sufficient size which is then able to attract gas, if available in the region of its formation.
 
2
Some readers may want to consult Lakes (2009), pg. 4 or Müller and Müller (2009), pg. 370 for more information.
 
3
The label \(\tau = 0\) in Figs. 3, 4 is to be understood in the sense \(\tau \approx 0\) (i.e., very small but not equal to zero). A more detailed discussion of this degenerated case can be found in Müller and Weiss (2016).
 
4
The interested reader is referred to Müller and Weiss (2016).
 
5
The interested reader may want to consult Müller and Weiss (2016) for further information.
 
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Metadata
Title
A Closed-Form Solution for a Linear Viscoelastic Self-gravitating Sphere
Authors
Wolfgang H. Müller
Elena N. Vilchevskaya
Copyright Year
2016
Publisher
Springer Singapore
DOI
https://doi.org/10.1007/978-981-10-0959-4_5

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