Granular gases are composed of macroscopic bodies kept in motion by an external
energy source such as a violent shaking. The behaviour of such systems is
quantitatively different from that of ordinary molecular gases: due to the size of
the constituents, external fields have a stronger effect on the dynamics and, more
importantly, the kinetic energy of the gas is no longer a conserved quantity. The
key role of the inelasticity of collisions has been correctly appreciated for about
fifteen years, and the ensuing consequences in terms of phase behaviour or transport
properties studied in an increasing and now vast body of literature.
The purpose of this book is to help the newcomer to the field in acquiring the
essential theoretical tools together with some numerical techniques. As emphasized
by the authors—who were among the pioneers in the domain— the content could be
covered in a one semester course for advanced undergraduates, or it could be
incorporated in a more general course dealing with the statistical mechanics of
dissipative systems.
The book is self-contained, clear, and avoids mathematical complications. In order
to elucidate the main physical ideas, heuristic points of views are sometimes
preferred to a more rigorous route that would lead to a longer discussion. The 28
chapters are short; they offer exercises and worked examples, solved at the end of
the book. Each part is supplemented with a relevant foreword and a useful summary
including take-home messages. The editorial work is of good quality, with very few
typographical errors.
In spite of the title, kinetic theory stricto sensu is not the crux of the
matter covered. The authors discuss the consequences of the molecular chaos
assumption both at the individual particle level and in terms of collective
behaviour. The first part of the book addresses the mechanics of grain collisions.
It is emphasized that considering the coefficient of restitution ε —a central
quantity governing the inelasticity of inter-grain encounters—as velocity
independent is inconsistent with the mechanical point of view. An asymptotic
expression for the impact velocity dependence of ε is therefore derived for
visco-elastic spheres. The important inelastic Boltzmann equation is introduced in
part II and the associated velocity distribution characterized for a force-free
medium (so-called free cooling regime). Transport processes can then be analyzed in
part III at the single particle level, and part IV from a more macroscopic
viewpoint. The corresponding Chapman–Enskog-like hydrodynamic approach is worked out
in detail, in a clear fashion. Finally, the tendency of granular gases to develop
instabilities is illustrated in part V where the hydrodynamic picture plays a
pivotal role.
This book clearly sets the stage. For the sake of simplicity, the authors have
discarded some subtle points, such as the open questions underlying the hydrodynamic
description (why include the temperature among the hydrodynamic modes, and what
about the separation of space and time scales between kinetic and hydrodynamic
excitations?). Such omissions are understandable. To a certain extent however, the
scope of the book is centered on previous work by the authors, and I have a few
regrets. Special emphasis is put on the (variable ε) visco-elastic model, which
enhances the technical difficulty of the presentation. On the other hand, the
important physical effects including scaling laws, hydrodynamic behaviour and
structure formation, can be understood in two steps, from the results derived within
the much simpler constant ε model, allowing subsequently $\varepsilon$ to depend on
the granular temperature. The authors justify their choice with the inconsistency of
the constant ε route. The improvements brought by the visco-elastic model remain to
be assessed, since the rotational degrees of freedom, discarded in the book, play an
important role and require due consideration of both tangential and normal
restitution coefficients, that are again velocity dependent. This seems to be the
price of a consistent approach, which does not lend itself to much insight. In
addition, the behaviour of driven systems is not addressed, whereas in the realm of
granular media, force-free systems are the exception rather than the rule. The
differences between constant ε and visco-elastic models is presumably less
pronounced in the driven case. Study of driven systems also reveals that the
rheology of granular gases is intrinsically non-Newtonian, which is a key feature.
Finally, the powerful direct simulation Monte Carlo technique is not described,
whereas it is an important tool, particularly relevant for the physics of the
Boltzmann equation, and straightforward to implement in its simplest version. N
Brilliantov and T Pöschel concentrate on the (equally relevant) molecular dynamics
method instead.
In conclusion, the book fills a gap in the field. The companion webpage from where
molecular dynamics and symbolic algebra programs can be downloaded is also
useful.