Abstract
In this chapter, we study the properties of strong supersonic explosions leading to a blast wave propagation. The so-called Sedov–Taylor–von Neumann (S–T–vN) approach is followed, which consists in finding a formal or numerical approximation in a self-similar schematization of the problem. Once the spherical propagation front time dependence has been found via a dimensional reasoning, the values of the internal quantities are determined by the solution of a system of ODEs. Application to the determination of the unknown amount of energy released by a bomb or a Supernova (SN) follows.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Notes
- 1.
Note that the binding energy usually referred to in the literature as the amount of energy to give to a specific nucleus to disperse all its elements (nucleons) is the absolute value of the nucleus energy at rest.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2023 The Author(s), under exclusive license to Springer Nature Switzerland AG
About this chapter
Cite this chapter
Capuzzo Dolcetta, R.A. (2023). Blast Waves. In: Physics of Fluids. UNITEXT for Physics. Springer, Cham. https://doi.org/10.1007/978-3-031-30750-8_5
Download citation
DOI: https://doi.org/10.1007/978-3-031-30750-8_5
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-031-30749-2
Online ISBN: 978-3-031-30750-8
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)