Institut : Neumann R & D Engineering, Düsseldorf

An excitation effect that could be involved in the dark matter phenomenon

Fachbereich : Physik

wissenschaftliche Forschungsarbeit

von

Eugen Mihailescu

Abgabedatum : 2005

Kommentar allg.:
Die wissenschaftliche Forschungsarbeit wurde z.T. unter der Mitwirkung des Institutes für Thermodynamik an der Universität der Bundeswehr Hamburg durchgeführt (s. Inhalt der Arbeit und technisches Gutachten) und könnte für eine breite Leserschaft von Interesse sein. Der Autor betrachtet das Vermitteln neuer Forschungsergebnisse als vorrangig vor finanziellen Interessen und würde trotz des Themas und der Länge der Forschungsarbeit einen Verkaufspreis von 10 – 15 Euro als angemessen betrachten. Die Entscheidung hierzu unterliegt jedoch naturgemäß dem Verlag. Der Leiter des Institutes für Thermodynamik an der Universität der Bundeswehr Hamburg, Prof. Kabelac, verzichtet darauf als Co-Autor der Arbeit aufzutreten, bat mich jedoch im Bereich „acknowledgments“ genannt zu werden. Dieser Bitte habe ich entsprochen.

An excitation effect that could be involved in the dark matter phenomenon Abstract. The dark matter phenomenon is known since 1933 and it correlates with the formation and the stability of galaxies and other large-scale structures. In the year 1933 Fritz Zwicky discovered a stabilization effect connected to the Coma cluster of galaxies [Zwicky, F. Helv. Phys. Acta 6, 110 – 127 (1933)]. The first interpretation of this stabilization effect leaded to the hypothesis of dark matter particles that could correlate with a gravitational effect and that could be involved in the stability of galaxies. Despite the fact that the stability of galaxies and galaxy clusters is known since more then 70 years, no consistent experimental data is presently known to support the hypothesis of dark matter particles. The assumed dark matter particles are presently not yet detected. The main experiment regarding dark matter particles of the year 2004, respectively the CDMS II experiment [D.S. Akerib et al., Phys. Rev. Lett. 93, 211301 (2004)] could not confirm the existence of dark matter particles, respectively of WIMPs (weakly interacting massive particles).

Following an alternative interpretation of the stabilization effect performed by galaxies and other large-scale structures connected to a boson field, a special excitation effect was found. This special excitation effect occurs without any presently known form of excitation and it is detectable in connection with different kind of material samples inside the cavity of a black body during laboratory experiments as well as during experiments performed outdoors in free nature. This excitation effect is followed by a regular pattern of emission in the spectral range of 160 – 630 nm at 273 – 300 K. The regular pattern of emission is uninterrupted detectable for at least 7 days in connection with samples made of granite and granodiorite.

Table of contents

1. Introduction

2. An alternative theoretic concept of the dark matter phenomenon
2.1. An overview on the dark matter phenomenon
2.2. An alternative theoretic concept of the dark matter phenomenon based on a boson field

3. The both experimental hypotheses of an excitation effect performed by a boson field eventual involved in the dark matter phenomenon

4. The experimental basic idea

5. The experimental assembly

6. The experimental verification of the presented hypotheses
6.1. The exposure of selected material samples to the verified boson field
6.1.1. Experimental results
6.1.2. The main findings
6.2. The exposure of material structures to the emission of particles from a force field amplification knot of the verified boson field
6.2.1. The exposure of selected material samples to the emission of particles from a force field amplification knot of the verified boson field
6.2.1.1. Experimental results
6.2.2. The exposure of the experimental assembly to the emission of particles from a force field amplification knot of the verified boson field
6.2.2.1. Experimental results
6.2.3. The main findings

7. Experimental uncertainties

8. Discussion
8.1. Backgrounds
8.2. The eventual influence of low level natural radioactivity on the founded UV-VIS emission inside the cavity of the experimental assembly
8.3. Delimitation of the UV-VIS emission inside the cavity of the experimental assembly against thermal radiation and luminescence (phosphorescence, fluorescence, etc.)

9. Conclusions

10. The next steps

Acknowledgements

Literaturverzeichnis / References
Anhang A. Figures captions [12 figures (8 color and 4 black and white) and 6 tables]
Anhang B. Expertise regarding the founded excitation effect (german) – enclosed : 8 color figures

Specifications:
- the expertise was performed at the Institute for Thermodynamics of the University of the Federal Armed Forces Hamburg, Germany
- the expertise is regarding the presented excitation effect observed during an experiment performed outdoors in free nature for 56h
- Content: 1. Einführung
2. Die Berechnung der zu erwartenden Strahlungsleistung in einem Hohlraum
3. Die Berechnung der zu erwartenden Counts durch den Detektor
4. Versuchsauswertung
5. Anlagen : Prüfung des dark count Verhaltens des eingesetzten Detektors

Abstract

The dark matter phenomenon is known since 1933 and it correlates with the formation and the stability of galaxies and other large-scale structures. In the year 1933 Fritz Zwicky discovered a stabilization effect connected to the Coma cluster of galaxies [Zwicky, F. Helv. Phys. Acta 6, 110 – 127 (1933)]. The first interpretation of this stabilization effect leaded to the hypothesis of dark matter particles that could correlate with a gravitational effect and that could be involved in the stability of galaxies. Despite the fact that the stability of galaxies and galaxy clusters is known since more then 70 years, no consistent experimental data is presently known to support the hypothesis of dark matter particles. The assumed dark matter particles are presently not yet detected. The main experiment regarding dark matter particles of the year 2004, respectively the CDMS II experiment [D.S. Acerb et al., Phys. Rev. Let. 93, 211301 (2004)] could not confirm the existence of dark matter particles, respectively of WIMPs (weakly interacting massive particles).

Following an alternative interpretation of the stabilization effect performed by galaxies and other large-scale structures connected to a boson field, a special excitation effect was found. This special excitation effect occurs without any presently known form of excitation and it is detectable in connection with different kind of material samples inside the cavity of a black body during laboratory experiments as well as during experiments performed outdoors in free nature. This excitation effect is followed by a regular pattern of emission in the spectral range of 160 – 630 nm at 273 – 300 K. The regular pattern of emission is uninterrupted detectable for at least 7 days in connection with samples made of granite and granodiorite.

1. Introduction
The dark matter phenomenon correlates with the formation and the stability of large-scale structures like galaxies. Independent and probably the most compelling evidence for the dark matter phenomenon comes from observations of the cosmic microwave background (CMB). Its discovery in 1965 by Penzias and Wilson [1] established modern cosmology. Recently the NASA Wilkinson Anisotropy Probe (WMAP) has provided high-resolution maps of the CMB [2,3].

The latest CMB data are indicating that the universe possesses a density ΩDM of 0.23 that correlates with the dark matter phenomenon and a density ΩM of 0.04 that correlates with ordinary baryonic matter. Presently it seems that the Universe is made up as follows: 23 % correlating with the dark matter phenomenon, 4 % correlating with ordinary baryonic matter and 73 % correlating with the dark energy phenomenon.

In the year 1992 the Cosmic Background Explorer (COBE) satellite measured slight fluctuations in the CMB at a level of one part in 100,000 [4]. This CMB anisotropy had been apparently involved in the formation of large-scale structures, respectively had been apparently the seeds for the gravitational clustering of baryonic matter.

This small variations in the temperature of the CMB detected by the COBE satellite, as shown in Fig. 1, are indicating a structuring effect connected with the dark matter phenomenon. The dark matter phenomenon correlates apparently with at least two different effects on baryonic matter, the well known stabilization effect on galaxies and on other large-scale structures and the formation effect for cosmic structures.

High-resolution observation of the CMB fluctuations provided in the last decade detailed information for cosmological models and theoretical concepts are now emerging for the formation of cosmic structure and for the evolution of the Universe. The crucial ingredients of this theories are the dark matter phenomenon and dark energy phenomenon.

2. An alternative theoretic concept of the dark matter phenomenon
2.1. An overview on the dark matter phenomenon

Presently two different theories are connected with the dark matter phenomenon.

One of this theories is based on the cold dark matter concept (CDM). This theory assumes the existence of weakly interacting massive particles, or WIMPS, with a mass of about 100 to 1,000 times the mass of a proton, that would be involved in the dark matter phenomenon and that would lead to a gravitational effect. In a Universe dominated by cold dark matter, respectively by WIMPS, the large – scale structure formation would have started with the forming of galaxies. Galaxies clustered then into larger structures, respectively in galaxy clusters and superclusters. Most of cold dark matter would thereby be concentrated in the great voids, outside of galaxy superclusters and strings. This scenario of formation of cosmic structures is known as a “bottom – up” structure formation scenario.

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