#### Preface

It is a great pleasure for me that I am in charge to write the preface to this book in honor
of my highly estimated colleague Prof. Dr. J. A. Maruhn to celebrate his retirement. The
broad span of contributions collected here demonstrates the versatility and the great public
visibility of Joachim Maruhn. One can read off from the collection that he has worked
in many areas of theoretical physics: structure of exotic nuclei, large-amplitude nuclear
dynamics, and plasmas with high energy density. The entrance to each one of these fields
was novel and pioneering computational development. To see this in more detail, we have to
go back to the beginnings of his career. I happened to be grown up in the same institute as
Joachim Maruhn, namely in the institute for Theoretical Physics of the Johann-Wolfgang-
Goethe university Frankfurt under Prof. Dr. W. Greiner. At this time around 1970, Joachim
Maruhn was the first to dig deep into the architecture of those days mainframe computers.
He had the patience to scrutinize all their bulky manuals, did even understand them, and
was able to squeeze the most out of these cumbersome monsters. I remember standing at
the controller room of the “huge” Univac 1108 of this time while his codes were running. All
of a sudden the tapes moved miraculously forth and back something which never happened
with our other codes. Joachim Maruhn was the one to grasp the obnoxious instructions to
speak to these devices and so he managed to write code for problems which were considered
extraordinarily bulky at this time when the RAM covered as much as 64 Kwords. At a later
occasion, I watched him installing one of the first affordable local computers by typing in
machine instructions in hexadecimal code, again very close to the hardware architecture.
These examples should not mislead the reader to the false impression that Joachim Maruhn
were a computer freak having lost contact to the real world. Yes, it is true that he has a sixth
sense for computing. But he keeps that in the proper balance and considers it as useful tool
to reach physics goals. Many of his developments started indeed as computational progress,
but all of them ended up in long standing and fruitful physics projects as can be read off
from his list of publications and from the articles in this book.

As his first master-piece, Joachim Maruhn delivered in the early 1970ies the Fortran
code for the Two-Center Shell-Model, a code which was used since for decades by many
colleagues all over the world for theoretical research on nuclear fusion, fission, and multi-
fragmentation. Not much later, he was one of the first to enter the field of simulating nuclear
dynamics fully microscopically on the basis of the time-dependent Hartree-Fock (TDHF)
method. This was a rather daring enterprise at that time where computer capacities were
comparatively poor. I remember wise colleagues shaking their head and recommending
rather to do something useful, because they could not believe that numerical capacities will
evolve so rapidly as they did. Today, we see that realistic TDHF simulations under varied
conditions are feasible and widely used. Thanks to the foreseeing, pioneering work of Joachim
Maruhn and similarly brave colleagues, we dispose now of long standing coding experience
and a variety of useful tools for these (still) demanding TDHF simulations. Besides that, this
experience has been successfully transferred to related areas in nuclear physics, particularly
the adiabatic description of nuclear collective motion and fission in a fully self-consistent
fashion. Also in the 1970ies, Joachim Maruhn entered the field of dynamical simulations
in plasma physics. And again, he managed to start novel developments which were at
this time at the edge of feasibility, if not beyond. In the meantime, the codes have been
employed successfully for many research projects up to now, particularly for the numerically
demanding plasma state under the extreme conditions of inertial fusion. Within these long
standing great development lines, there appeared often remarkable details. For example,
Joachim Maruhn composed a time- and memory-saving generator for FFT routines which
managed to generate automatically code for each grid size separately, so taking advantage of
trivial numbers (e.g. multiplication by 1) occurring for many cases, but always at different
places. To the best of my knowledge, this was the fastest FFT routine around for long time
until the modern libraries appeared, as e.g. FFTW, which, in fact, use similar strategies of
dedicated coding for given grid size. There are many others example for such fine details.
Quite generally, the itching limitations of former computers called for careful coding to use
resources as efficient as possible. Up to these days, Joachim Maruhn’s codes are exemplary
for excellent coding, readable, efficient and reliable. But again, coding was never considered
as an end in itself. It provided “merely” a sound basis for far reaching physics projects.
These project lines can be grouped in four main branches which will be briefly outlined
below.

The earliest achievement was the Two-Center Shell-Model (TCSM) which belongs to
the class of microscopic-macroscopic models. This kind of modeling was the method of
choice in the 1960ies and 70ies. At that time one could not dream of the later progress
of fully self-consistent models. Thus one tailored effective single-particle potentials (shell
models) following the physical intuition associated with nuclear collective motion and fis-
sion. Combining the quantum effects from the shell model with the well understood bulk
properties from the liquid-drop model provides a remarkably reliable description which is
still competitive today. The TCSM was a big step forward within this successful family of
microscopic-macroscopic models because it was the first one to work in a basis of single-
particle wavefunctions which cover the fragmentation of nuclear centers. This was achieved
by putting two harmonic oscillator potentials side by side and cutting them at the crossing
point. This gives the model the freedom to handle any fragment shapes, however at the price
of making the numerical handling of the basis functions more involved which was a challenge
in the 1970ies. Since then, the TCSM with its great versatility has found widespread appli-
cations and remains even today a useful tool for first explorations of exotic fragmentation
channels.

Purely macroscopic modeling is used in the hydrodynamical code which Joachim Maruhn
developed since the mid 1970ies. Motivated was this by the upcoming heavy-ion facilities.
There was a need for an affordable simulation of the dynamics of violent heavy-ion collisions
up to including a pertinent description of nuclear shock waves. But later on, the hydro-
dynamical code found its major applications in a different field, namely plasma physics.
This was still related to heavy-ion facilities, here, however, related to a totally different use
of heavy-ion beams, namely for the generation of extremely hot and dense plasma states.
The fact that the university Frankfurt close to GSI Darmstadt allowed an extremely fruitful
collaboration between Joachim Maruhn’s plasma group and experimentalists at GSI up to
these days. The theoretical simulations are here deeply connected with application. They
serve as crucial instruments to understand and design experiments.

Also in the mid 1970ies appeared on the horizon first fully self-consistent microscopic
nuclear mean-field models which allowed a reliable description of nuclear properties. This
triggered a storm of new developments in modeling nuclear structure and dynamics. Time-
dependent Hartree-Fock (TDHF) is the most far fetched application in this scenario. Joachim
Maruhn was one of the forerunners in this first wave of TDHF development. The early TDHF
studies allowed to gain insight into the basic mechanisms of nuclear collisions as flow pattern
or the threshold between fusion and inelastic scattering.

The limitations of former days computers hindered to proceed with TDHF to realis-
tic simulations. However, the elaborate griding techniques developed for TDHF could be
recycled for many useful applications in nuclear structure physics and adiabatic nuclear dy-
namics. Joachim Maruhn exploited that extensively which led to a rich series of publications
on exotic nuclei, particularly super-heavy elements. A crucial issue was here the prediction
of stability which is related to a reliable estimate of fission barriers. Mind that these stud-
ies deal with far extrapolations. This raises questions about the reliability of the effective
density functionals used in self-consistent nuclear models. Careful as he is, Joachim thus
focused very much on studying critically the parametrizations of nuclear density functionals,
the relativistic mean-field model as well as the non-relativistic Skyrme-Hartree-Fock func-
tional. These extensive investigations have eventually pointed out quite clearly the regimes
of nuclei and observables which can be predicted reliably well and those which have to
be taken with care. These results have, furthermore, served to improve the self-consistent
models and its parametrization.

Meanwhile, computing capacities have evolved so rapidly that one can actually perform
those realistic TDHF simulations which we were dreaming in the 1970ies. This led to a
remarkable revival of TDHF studies and, of course, Joachim Maruhn is heavily involved
in this second round TDHF. It is now possible to do away with all symmetry restrictions
which hampered early TDHF codes and to run unbiased simulations. This allows, e.g., to
run collisions of truly heavy ions (as Pb or U) and to spend sizable computing effort or
detailed analysis of the results which, in turn, inspired a couple of novel investigations. One
example is the detailed microscopic computation of cross sections for over-barrier fusion
of heavy nuclei. Another example is the tracking of collisional dynamics in a phase space
picture with the help of the six-dimensional Wigner transformation which gives insight,
e.g., into dynamical transfer processes or into dissipation mechanisms at work in TDHF.
Really huge systems were attacked in the realm of astro-physics when simulating hot nuclear
matter under the typical conditions in a super-nova explosion. The various phases of nuclear
matter which had been previously assessed in symmetry-restricted stationary models can
now be probed in a truly dynamical situation which yields additional information on their
structure, stability and prevalence. One of the exciting results is that nuclear matter can
form under certain conditions a gyroid structure which is a curved, interwoven network of
matter and voids. This is surely not the end of the TDHF revival. There are still many
promising investigations in the queue as, e.g., an improved description of fission and a better
understanding (or modeling) of dissipation. I am confident that Joachim Maruhn continues
to contribute to these studies.

Thus far, I have reviewed Joachim Maruhn from a purely scientific perspective. But that
leaves an incomplete picture. Joachim Maruhn was not only digging deep into computers
and publishing good papers all day. He was for long time appointed as Professor at the
Johann-Wolfgang-Goethe university Frankfurt and as such predominantly a teacher. He
took it very serious and delivered excellent lectures. His list of publications shows a couple
of textbooks and looking at them gives an impression of his clear and crisp explanations.
Students appreciated that very much and honored him with the price for good teaching,
probably that achievement of which Joachim Maruhn is most proud of. And this pride
in itself demonstrated how much he focused on teaching students. More than that, he
cared for them, listening to their concerns and often inventing creative solutions for sticky
administrative blockades with examinations and certificates. Not surprising that he was
asked to serve the faculty as Dean of Students, a time-consuming burden which he fulfilled
with patience and equanimity. He did it fully hearted and right with the same commitment
as his scientific enterprises.

I close with a personal remark. We started common projects in the late 1970ies, at the
time when he came back to Frankfurt as Professor for Theoretical Physics. Since then we
continue close collaboration in nuclear structure physics and TDHF. I am very thankful for
all we could work out together, for his advice and for is inspiration. I wish Joachim Maruhn
that he can stay in science for many further years, supplying more of his interesting findings,
and, somewhat egoistically, that we can enjoy further common projects.

#### List of Contributors

##### Editor(s):

**Yoritaka Iwata **

School of Science

The University of Tokyo, Hongo 7-3-1, 113-0033 Tokyo,

Japan