Kaatopaikkakaasun hyötykäyttömahdollisuudet Anjalankosken Ekoparkissa

Kaatopaikalle sijoitetut biohajoavat orgaaniset jätteet muodostavat jätetäytön hapettomissa olosuhteissa kaatopaikkakaasua, joka koostuu pääasiassa metaanista ja hiilidioksidista. Kaatopaikkakaasun sisältämän metaanin takia, kaasusisältää merkittävästi energiaa, joka on hyödynnettävissä eri tavoin. Tämän diplomityön tavoitteena oli tarkastella vaihtoehtoja Anjalankosken Keltakankaan kaatopaikoilla muodostuvan kaatopaikkakaasun hyödyntämiseksi. Tarkastellut vaihtoehdot tarjoavat ympäristöllisten hyötyjen lisäksi liiketoiminnallista hyötyä Ekoparkissa toimiville yrityksille. Tutkimuksessa tehdyt laskelmatosoittivat, että työssä tarkastellut kaatopaikkakaasun hyötykäyttövaihtoehdot ovat sekä taloudellisesti että kaasun riittävyyden kannalta hyödynnettävissä. Esimerkiksi kaatopaikkakaasun hyödyntämisellä kaukolämmön tuotannossa voidaan kattaa noin kolmannes Anjalankosken vuotuisesta kaukolämmön tarpeesta. Kaatopaikkakaasun lietteen kuivauskapasiteetti kattaa Pohjois-Kymenlaaksossa muodostuvan jätevesilietteen käsittelytarpeen. Biopolttoaineen kuivauskapasiteetti on riittävä olemassa oleviin valmistuslaitosten tuotantokapasiteetteihin verrattuna. Myös perinteisillä sähkön- ja lämmöntuotantotekniikoilla voidaan kattaa Ekoparkin oma sähkön- ja lämmöntarve. Kaatopaikkavesien haihdutus ei tulosten perusteella ole sekä taloudellisesti että kaasun riittävyyden kannalta hyödynnettävissä. Tuhkan vitrifioinnissa haasteen muodostaa investointikustannuksen suuruus. Anjalankosken Ekoparkin yritykset voivat hyödyntää työn tuloksia uuden liiketoiminnan kehittämiseen. Lisäksi tuloksia voidaan hyödyntää soveltaen eri kokoluokan kaatopaikkojen kaatopaikkakaasujen hyötykäyttöä suunniteltaessa.

BoBo mixing meseasurement at Belle using dilepton events tagged with a soft pion

L'expérience Belle, située dans le centre de recherche du KEK, au Japon, est consacrée principalement à l'étude de la violation de CP dans le système des mésons B. Elle est placée sur le collisionneur KEKB, qui produit des paires Banti-B. KEKB, l'une des deux « usines à B » actuellement en fonction, détient le record du nombre d'événements produits avec plus de 150 millions de paires. Cet échantillon permet des mesures d'une grande précision dans le domaine de la physique du méson B. C'est dans le cadre de ces mesures de précision que s'inscrit cette analyse. L'un des phénomènes remarquables de la physique des hautes énergies est la faculté qu'a l'interaction faible de coupler un méson neutre avec son anti-méson. Dans le présent travail, nous nous intéressons au méson B neutre couplé à l'anti-méson B neutre, avec une fréquence d'oscillation _md mesurable précisément. Outre la beauté de ce phénomène lui-même, une telle mesure trouve sa place dans la quête de l'origine de la violation de CP. Cette dernière n'est incluse que d'une façon peu satisfaisante dans le modèle standard des interactions électro-faibles. C'est donc la recherche de phénomènes physiques encore inexpliqués qui motive en premier lieu la collaboration Belle. Il existe déjà de nombreuses mesures de _md antérieures. Celle que nous présentons ici est cependant d'une précision encore jamais atteinte grâce, d'une part, à l'excellente performance de KEKB et, d'autre part, à une approche originale qui permet de réduire considérablement la contamination de la mesure par des événements indésirés. Cette approche fut déjà mise à profit par d'autres expériences, dans des conditions quelque peu différentes de celles de Belle. La méthode utilisée consiste à reconstruire partiellement l'un des mésons dans le canal ___D*(D0_)l_l, en n'utilisant que les informations relatives au lepton l et au pion _. L'information concernant l'autre méson de la paire Banti-B initiale n'est tirée que d'un seul lepton de haute énergie. Ainsi, l'échantillon à disposition ne souffre pas de grandes réductions dues à une reconstruction complète, tandis que la contamination due aux mésons B chargés, produits par KEKB en quantité égale aux B0, est fortement diminuée en comparaison d'une analyse inclusive. Nous obtenons finalement le résultat suivant : _md = 0.513±0.006±0.008 ps^-1, la première erreur étant l'erreur statistique et la deuxième, l'erreur systématique.<br/><br/>The Belle experiment is located in the KEK research centre (Japan) and is primarily devoted to the study of CP violation in the B meson sector. Belle is placed on the KEKB collider, one of the two currently running "B-meson factories", which produce Banti-B pairs. KEKB has created more than 150 million pairs in total, a world record for this kind of colliders. This large sample allows very precise measurements in the physics of beauty mesons. The present analysis falls within the framework of these precise measurements. One of the most remarkable phenomena in high-energy physics is the ability of weak interactions to couple a neutral meson to its anti-meson. In this work, we study the coupling of neutral B with neutral anti-B meson, which induces an oscillation of frequency _md we can measure accurately. Besides the interest of this phenomenon itself, this measurement plays an important role in the quest for the origin of CP violation. The standard model of electro-weak interactions does not include CP violation in a fully satisfactory way. The search for yet unexplained physical phenomena is, therefore, the main motivation of the Belle collaboration. Many measurements of _md have previously been performed. The present work, however, leads to a precision on _md that was never reached before. This is the result of the excellent performance of KEKB, and of an original approach that allows to considerably reduce background contamination of pertinent events. This approach was already successfully used by other collaborations, in slightly different conditions as here. The method we employed consists in the partial reconstruction of one of the B mesons through the decay channel ___D*(D0_)l_l, where only the information on the lepton l and the pion _ are used. The information on the other B meson of the initial Banti-B pair is extracted from a single high-energy lepton. The available sample of Banti-B pairs thus does not suffer from large reductions due to complete reconstruction, nor does it suffer of high charged B meson background, as in inclusive analyses. We finally obtain the following result: _md = 0.513±0.006±0.008 ps^-1, where the first error is statistical, and the second, systematical.<br/><br/>De quoi la matière est-elle constituée ? Comment tient-elle ensemble ? Ce sont là les questions auxquelles la recherche en physique des hautes énergies tente de répondre. Cette recherche est conduite à deux niveaux en constante interaction. D?une part, des modèles théoriques sont élaborés pour tenter de comprendre et de décrire les observations. Ces dernières, d?autre part, sont réalisées au moyen de collisions à haute énergie de particules élémentaires. C?est ainsi que l?on a pu mettre en évidence l?existence de quatre forces fondamentales et de 24 constituants élémentaires, classés en « quarks » et « leptons ». Il s?agit là de l?une des plus belles réussites du modèle en usage aujourd?hui, appelé « Modèle Standard ». Il est une observation fondamentale que le Modèle Standard peine cependant à expliquer, c?est la disparition quasi complète de l?anti-matière (le « négatif » de la matière). Au niveau fondamental, cela doit correspondre à une asymétrie entre particules (constituants de la matière) et antiparticules (constituants de l?anti-matière). On l?appelle l?asymétrie (ou violation) CP. Bien qu?incluse dans le Modèle Standard, cette asymétrie n?est que partiellement prise en compte, semble-t-il. En outre, son origine est inconnue. D?intenses recherches sont donc aujourd?hui entreprises pour mettre en lumière cette asymétrie. L?expérience Belle, au Japon, en est une des pionnières. Belle étudie en effet les phénomènes physiques liés à une famille de particules appelées les « mésons B », dont on sait qu?elles sont liées de près à l?asymétrie CP. C?est dans le cadre de cette recherche que se place cette thèse. Nous avons étudié une propriété remarquable du méson B neutre : l?oscillation de ce méson avec son anti-méson. Cette particule est de se désintégrer pour donner l?antiparticule associée. Il est clair que cette oscillation est rattachée à l?asymétrie CP. Nous avons ici déterminé avec une précision encore inégalée la fréquence de cette oscillation. La méthode utilisée consiste à caractériser une paire de mésons B à l?aide de leur désintégration comprenant un lepton chacun. Une plus grande précision est obtenue en recherchant également une particule appelée le pion, et qui provient de la désintégration d?un des mésons. Outre l?intérêt de ce phénomène oscillatoire en lui-même, cette mesure permet d?affiner, directement ou indirectement, le Modèle Standard. Elle pourra aussi, à terme, aider à élucider le mystère de l?asymétrie entre matière et anti-matière.

Compact thermal storage: a-state-of-the-art review of experimental results

Thermal energy storage (TES) can increase the thermal energy effieresa, of a process by reusing the waste heat from industrial process, solar energy or other sources. There are different ways to store thermal energy: by sensible heat, by latest heat, by sorption process or by chemical reaction. This thesrs provides a-state-of-the-art review of the experimental performance of TES systems based on solid gas sorption process and chemical reactions. The importance of theses processes is that provides a heat loss free storage system with a high energy density.

Fabrication and characterization of silicon position sensitive particle detectors

Position sensitive particle detectors are needed in high energy physics research. This thesis describes the development of fabrication processes and characterization techniques of silicon microstrip detectors used in the work for searching elementary particles in the European center for nuclear research, CERN. The detectors give an electrical signal along the particles trajectory after a collision in the particle accelerator. The trajectories give information about the nature of the particle in the struggle to reveal the structure of the matter and the universe. Detectors made of semiconductors have a better position resolution than conventional wire chamber detectors. Silicon semiconductor is overwhelmingly used as a detector material because of its cheapness and standard usage in integrated circuit industry. After a short spread sheet analysis of the basic building block of radiation detectors, the pn junction, the operation of a silicon radiation detector is discussed in general. The microstrip detector is then introduced and the detailed structure of a double-sided ac-coupled strip detector revealed. The fabrication aspects of strip detectors are discussedstarting from the process development and general principles ending up to the description of the double-sided ac-coupled strip detector process. Recombination and generation lifetime measurements in radiation detectors are discussed shortly. The results of electrical tests, ie. measuring the leakage currents and bias resistors, are displayed. The beam test setups and the results, the signal to noise ratio and the position accuracy, are then described. It was found out in earlier research that a heavy irradiation changes the properties of radiation detectors dramatically. A scanning electron microscope method was developed to measure the electric potential and field inside irradiated detectorsto see how a high radiation fluence changes them. The method and the most important results are discussed shortly.

Development of advanced silicon radiation detectors for harsh radiation environment

This thesis describes the development of advanced silicon radiation detectors and their characterization by simulations, used in the work for searching elementary particles in the European Organization for Nuclear Research, CERN. Silicon particle detectors will face extremely harsh radiation in the proposed upgrade of the Large Hadron Collider, the future high-energy physics experiment Super-LHC. The increase in the maximal fluence and the beam luminosity up to 1016 neq / cm2 and 1035 cm-2s-1 will require detectors with a dramatic improvement in radiation hardness, when such a fluence will be far beyond the operational limits of the present silicon detectors. The main goals of detector development concentrate on minimizing the radiation degradation. This study contributes mainly to the device engineering technology for developing more radiation hard particle detectors with better characteristics. Also the defect engineering technology is discussed. In the nearest region of the beam in Super-LHC, the only detector choice is 3D detectors, or alternatively replacing other types of detectors every two years. The interest in the 3D silicon detectors is continuously growing because of their many advantages as compared to conventional planar detectors: the devices can be fully depleted at low bias voltages, the speed of the charge collection is high, and the collection distances are about one order of magnitude less than those of planar technology strip and pixel detectors with electrodes limited to the detector surface. Also the 3D detectors exhibit high radiation tolerance, and thus the ability of the silicon detectors to operate after irradiation is increased. Two parameters, full depletion voltage and electric field distribution, is discussed in more detail in this study. The full depletion of the detector is important because the only depleted area in the detector is active for the particle tracking. Similarly, the high electric field in the detector makes the detector volume sensitive, while low-field areas are non-sensitive to particles. This study shows the simulation results of full depletion voltage and the electric field distribution for the various types of 3D detectors. First, the 3D detector with the n-type substrate and partial-penetrating p-type electrodes are researched. A detector of this type has a low electric field on the pixel side and it suffers from type inversion. Next, the substrate is changed to p-type and the detectors having electrodes with one doping type and the dual doping type are examined. The electric field profile in a dual-column 3D Si detector is more uniform than that in the single-type column 3D detector. The dual-column detectors are the best in radiation hardness because of their low depletion voltages and short drift distances.

Cosmic censorship in two-dimensional gravity

A weak version of the cosmic censorship hypothesis is implemented as a set of boundary conditions on exact semiclassical solutions of two-dimensional dilaton gravity. These boundary conditions reflect low-energy matter from the strong coupling region and they also serve to stabilize the vacuum of the theory against decay into negative energy states. Information about low-energy incoming matter can be recovered in the final state but at high energy black holes are formed and inevitably lead to information loss at the semiclassical level.

The star forming region Monoceros R2 as a gamma-ray source

After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood. Aims: The aim of this paper is to assess the possibility of the Fermi gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2. Methods: A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios. Results: We confirm the 2FGL J0607.5-0618c detection with improved confidence over the Fermi two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source.

Confirmation of persistent radio jets in the microquasar LS 5039

We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS 5039 discovered by Paredes et al. (2000) with the VLBA. The new observations confirm the presence of an asymmetric two-sided jet reaching up to 1000 AU on the longest jet arm. The results suggest a bending of the jets with increasing distance from the core and/or precession. The origin and location of the high-energy gamma-ray emission associated with the system is discussed and an estimate of the magnetic field at the base of the jet given. Our results suggest a well collimated radio jet. We also comment on new observing strategies to be used with satellites and forthcoming detectors, since this persistent source appears to be a rather good laboratory to explore the accretion/ejection processes taking place near compact objects.

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.

Observation of VHE γ-rays from Cassiopeia A with the MAGIC telescope

Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A Methods: The shell-type supernova remnant Cassiopeia A was observed with the 17 m MAGIC telescope between July 2006 and January 2007 for a total time of 47 h. Results: The source was detected above an energy of 250 GeV with a significance of 5.2σ and a photon flux above 1 TeV of (7.3 ± 0.7_stat ± 2.2_sys) × 10-13 cm-2s-1. The photon spectrum is compatible with a power law dN/dE ∝ E-Γ with a photon index Γ = 2.3 ± 0.2_stat ± 0.2_sys. The source is point-like within the angular resolution of the telescope.

Gamma-ray emission from microquasars: a numerical model for LSI+61º303

We explore the possible association between the microquasar LSI +61°303 and the EGRET source 2CG 135+01/3EG J0241+6103 by studying, with a detailed numerical model, whether this system can produce the emission and the variability detected by EGRET (>100 MeV) through inverse Compton (IC) scattering. Our numerical approach considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet, interacting with both the radiation and the magnetic fields, taking into account the Thomson and Klein-Nishina regimes of interaction. Our results reproduce the observed spectral characteristics and variability at γ-rays, thus strengthening the identification of LSI +61°303 as a high-energy γ-ray source.

Readout schemes for low noise single-photon avalanche diodes fabricated in conventional HV-CMOS technologies

Three different pixels based on single-photon avalanche diodes for triggered applications, such as fluorescence lifetime measurements and high energy physics experiments, are presented. Each pixel consists of a 20µm x 100µm (width x length) single photon avalanche diode and a monolithically integrated readout circuit. The sensors are operated in the gated mode of acquisition to reduce the probability to detect noise counts interferring with real radiation events. Each pixel includes a different readout circuit that allows to use low reverse bias overvoltages. Experimental results demonstrate that the three pixels present a similar behaviour. The pixels get rid of afterpulses and present a reduced dark count probability by applying the gated operation. Noise figures are further improved by using low reverse bias overvoltages. The detectors exhibit an input dynamic range of 13.35 bits with short gated"on" periods of 10ns and a reverse bias overvoltage of 0.5V. The three pixels have been fabricated in a standard HV-CMOS process.

MAGIC TeV Gamma-Ray Observations of Markarian 421 during Multiwavelength Campaigns in 2006

Wide-range spectral coverage of blazar-type active galactic nuclei is of paramount importance for understanding the particle acceleration mechanisms assumed to take place in their jets. The Major Atmospheric Gamma Imaging Cerenkov (MAGIC) telescope participated in three multiwavelength (MWL) campaigns, observing the blazar Markarian (Mkn) 421 during the nights of April 28 and 29, 2006, and June 14, 2006. Aims. We analyzed the corresponding MAGIC very-high energy observations during 9 nights from April 22 to 30, 2006 and on June 14, 2006. We inferred light curves with sub-day resolution and night-by-night energy spectra. Methods. MAGIC detects γ-rays by observing extended air showers in the atmosphere. The obtained air-shower images were analyzed using the standard MAGIC analysis chain. Results. A strong γ-ray signal was detected from Mkn 421 on all observation nights. The flux (E > 250 GeV) varied on night-by-night basis between (0.92±0.11) × 10-10 cm-2 s-1 (0.57 Crab units) and (3.21±0.15) × 10-10 cm-2 s-1 (2.0 Crab units) in April 2006. There is a clear indication for intra-night variability with a doubling time of 36± min on the night of April 29, 2006, establishing once more rapid flux variability for this object. For all individual nights γ-ray spectra could be inferred, with power-law indices ranging from 1.66 to 2.47. We did not find statistically significant correlations between the spectral index and the flux state for individual nights. During the June 2006 campaign, a flux substantially lower than the one measured by the Whipple 10-m telescope four days later was found. Using a log-parabolic power law fit we deduced for some data sets the location of the spectral peak in the very-high energy regime. Our results confirm the indications of rising peak energy with increasing flux, as expected in leptonic acceleration models.

Studying the non-thermal lobes of IRAS 16547-4247 through a multi-wavelength approach

In recent years, massive protostars have turned out to be a possible population of high-energy emitters. Among the best candidates is IRAS 16547-4247, a protostar that presents a powerful outflow with clear signatures of interaction with its environment. This source has been revealed to be a potential high-energy source because it displays non-thermal radio emission of synchrotron origin, which is evidence of relativistic particles. To improve our understanding of IRAS 16547-4247 as a high-energy source, we analyzed XMM-Newton archival data and found that IRAS 16547-4247 is a hard X-ray source. We discuss these results in the context of a refined one-zone model and previous radio observations. From our study we find that it may be difficult to explain the X-ray emission as non-thermal radiation coming from the interaction region, but it might be produced by thermal Bremsstrahlung (plus photo-electric absorption) by a fast shock at the jet end. In the high-energy range, the source might be detectable by the present generation of Cherenkov telescopes, and may eventually be detected by Fermi in the GeV range.

Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020

Context. There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to identify the physical counterpart, given the uncertainty in the source location and extension. Aims. This work carries out a thorough multi-wavelength study of the unidentified, very high energy source HESS J1858+020 and its environs. Methods. We have performed Giant Metrewave Radio Telescope observations at 610 MHz and 1.4 GHz to obtain a deep, low-frequency radio image of the region surrounding HESS J1858+020. We analysed archival radio, infrared, and X-ray data as well. This observational information, combined with molecular data, catalogue sources, and a nearby Fermi gamma-ray detection of unidentified origin, are combined to explore possible counterparts to the very high energy source. Results. We provide with a deep radio image of a supernova remnant that might be related to the GeV and TeV emission in the region. We confirm the presence of an H ii region next to the supernova remnant and coincident with molecular emission. A potential region of star formation is also identified. We identify several radio and X-ray sources in the surroundings. Some of these sources are known planetary nebulae, whereas others may be non-thermal extended emitters and embedded young stellar objects. Three old, background Galactic pulsars also neighbour HESS J1858+020 along the line of sight. Conclusions. The region surrounding HESS J1858+020 is rich in molecular structures and non-thermal objects that may potentially be linked to this unidentified very high energy source. In particular, a supernova remnant interacting with nearby molecular clouds may be a good candidate, but a star forming region, or a non-thermal radio source of yet unclear nature, may also be behind the gamma-ray source. The neighbouring pulsars, despite being old and distant, cannot be discarded as candidates. Further observational studies are needed, however, to narrow the search for a counterpart to the HESS source.