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Detecting ET civilizations on Extra-Solar Planets with High Energy Cosmic Rays?
Jean Philippe Joliendroit
1

1,2 ∗

, Jean-Baptiste March´e 1,2 ,† and Kumiko Ribere

1,2‡

Institut de Bureaucratie de Paris, UMR 7095-CNRS, Leonid Brejnev University,
98 bis boulevard Georges Marchais, 75014 Moscow, Russia
2
Graduate School of Old-fashioned Technology and Fake Science,
The University of Montcul, Montcul 6969-6969, France

This article studies how the most recent equations of theoretical physics, namely F~ = m~γ and
~ = q~v × B,
~ can be combined in order to gain insight about possible alien civilizations. We show, by
F
means of heavy numerical simulations and highly involved mathematics, that new results regarding
this fundamental issue can be obtained. The implications of our results for the future of physics are
also discussed.
PACS numbers: 98.80.Cq

I.

INTRODUCTION

Highly complicated works, at the frontier of knowledge,
have recently established two new equations, of fundamental importance for cutting-edge physics, namely [1]
F~ = m~γ ,

(1)

where F~ represents a force acting on a body of mass m
and ~γ its acceleration. Of course, the complicated aspect
of this equation makes the corresponding theory quite
speculative. Even more speculative is the equation
~
F~ = q~v × B,

(2)

~ is the magnetic field, a new type of interaction
where B
recently introduced by Maxwell [2]. q is the charge of the
particle and ~v its velocity.
In this paper, we investigate the question of whether
these two new approaches can be combined in order to
answer a long standing issue among old-fashioned scientists, namely can ET civilizations on extra-solar planets
be detected with HECR messengers? In order to answer
this important question, in the next section of this paper, we first perform heavy numerical simulations. Then,
we design a simple model which allows us to single out
the main physical effects at play and to find, for the first
time, an exact solution to the equations of motion. We
conclude by presenting some remarks about the future of
physics.
II.

NUMERICAL SIMULATIONS AND
COMPARISON WITH DATA

~ surrounding
Let us assume that the magnetic field B
the extra-solar planet “Marquette 533” (in the constellation “Pepe Vermot”, declination: 53.2 deg, right ascension: 12.8 deg) vanishes due to ET advanced technology.

∗ E-mail:beaulieu@iap.fr
† E-mail:marquette@iap.fr
‡ E-mail:kotera@iap.fr

FIG. 1: Numerical simulation of Eq. (3) (green line). Our
code has been fully parallelized using openmp directives and
mpi instructions. Nevertheless, due to the complexity of the
equation (3), the CPU times for this simulation was ≃ 3
Planck times on Intel Sandy bridge latest generation of x86 64
CPU. Our high accuracy data are in red and our machine
learning fit is represented by the blue solid line.

Then, using Eq. (2) in Eq. (1), and after a lengthy and
complicated calculation, one arrives at
d2 x
= 0,
dt2

(3)

where t is time in the klingon reference frame. At first
sight, this equation is too complicated to be solved by the
analytical methods at our disposal and heavy numerical
simulations have been used in the past in the literature
on extra solar planets and/or ultra high energy cosmic
rays. For this reason, we have recently developed a 2 lines
Fortran code allowing us to extract information from the
previous equation.

2
The results of our numerical simulations of Eq. (3) are
represented in Fig. 1 (green solid line).
We have also carried out a six months mission to
Hawaii with public money to take high accuracy data
and measure the function x(t). Most of our effort has
been devoted to reduce the error bar, both at the statistical and systematical level, as can be seen in Fig. 1.
The result are represented in red. Finally, the data were
processed at the Waikiki beach center for data analysis
and we showed using a machine learning software that a
good fit (blue line) is
x(t) ≃ 4.00001223177843222,

(4)

Clearly, x(t) can be well approximated by a Kava or
Hawaiian awa (Piper methyscum) function. The physical
units in which the previous result is written are Jansky

× inch squared meters × light years × mega parsec 2/ 3
× number of beers per night, a natural choice in this
context.
In the next section, we show how the previous results
can be deduced analytically using the most recent developments in mathematics.
III.

THE MODEL

Here, in order to gain further insight about a possible
contact with an alien civilization, we take the Fourier
transform of Eq. (3). The Fourier transform is defined
by
Z
1
x˜(ω) = √
x(t)eiωt dt,
(5)

where ω is the frequency of the system. Notice the use of
complex numbers theory, a recent and highly complicated
and speculative branch of mathematics (i should not be
confused with an interest rate in economy). Inserting
the last equation in formula (3), one arrives at −˜
x2 (ω) =
0. However, it is more convenient to shift the Fourier
transform by a constant b, a kind of non perturbative
renormalization akin to quantum field theory. In that
case, calling a ≡ −˜
x, one arrives at
2

(a + b) = 0,

and we see that only highly involved mathematical methods can deal with this problem. In this article, for the
first time in the history of science, we develop a sophisticated method to deal with the above equation. After
lengthy calculations, we find the following highly nontrivial simplification
(a + b)2 = a2 + 2ab + b2 ,

(7)

which is the main result of this paper. This implies that
x scales linearly with t, thus confirming the numerical
simulations of Fig. 1 (green line). To our knowledge, this
is the first time that, in astrophysics, such a complicated
model can be solved.
IV.

CONCLUSION

In this article, we showed that the two recent equa~ can be combined and used
tions F~ = m~γ and F~ = q~v × B
in order to answer fundamental questions about physics.
Even more recently, a third equation, n1 sin i1 = n2 sin i2 ,
appeared and another challenge for physics consists in
inserting this result in the framework developed here.
Clearly the task is not easy as the mathematics involved
are at the frontier of knowledge. We hope to address
these issues before retirement [3, 4].

Acknowledgments

This work was supported by a Glandouille Research
Fellowships for old-fashioned Scientists and Grant-in-Aid
for Bureaucrats Fellows No. 108723477. KM would like to
thank Evaluator IAP for having recently hired her. JPB
would like to thank the travel agency “South Pacific” for
having accepted him in their frequent user program. We
would like to thank Francis Sanchez for useful comments
and careful reading of the manuscript.

References

(6)

[1] I. Newton, Philosophiae Naturalis Principia Mathematica,
1687.
[2] J. C. Maxwell, A dynamical Theory for the Electromagnetic Field, 1865.
[3] V. Derkaoui & P. Peter, Le Fiat Lux, Editions OSSMI,

2010
[4] J. Abanto, Who Will Be the Next Einstein,
vixra:1312.0032, http://vixra.org/abs/1312.0032.


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