21. Oujda (Morocco) Fuses Astrophysics With Particle Physics And astrophysicists involved in highenergy particle and astro-physics research in fuseseemingly disparate fields as cosmic rays, dark matter from gravitational http://www.saao.ac.za/~wgssa/as6/guessoum.html

22. The Aim Of The Joint Astrophysics Division properties of the Universe such as the Hubble constant, the cosmological constant,the hadronic and the darkmatter densities. As ‘astro-physics’ 2 should http://www.europhysicsnews.com/full/12/article16/article16.html

Europhysics News (2001) Vol. 32 No. 6 The aim of the Joint Astrophysics Division Maurice Jacob Chairman of JAD T here is at present a thriving interface between physics and astronomy and the purpose of JAD is to respond to the need of the fast expanding community of scientists working in that domain by organising workshops and conferences and providing forums for discussion whenever needed. JAD should eventually become a grassroots partner for research organisations that try to co-ordinate their programmes as, for example the newly created AstroParticle Physics European Co-ordination (APPEC). In 2000, JAD organised the first ESA-CERN workshop on “Fundamental Physics in Space”, which was held at CERN [1]. The past and present chairmen invested much effort in helping to establish permanent links between ESA and CERN, and the two organisations have actually found several areas of fruitful collaboration. The Joint Astrophysics Division has two sections: one on “Solar Physics”, which has long existed and which organises a well-attended European conference in that domain every three years (Chairman: Jan Kuijpers, Nijmwegen);

23. PARTICLE PHYSICS FRIDAY APRIL 19 session 8 - astro-physics Astro-particle - Astrophysics(cont'd). 830, dark matter Searches, P. Baillon, EP Div - CERN. http://lemoigne.home.cern.ch/lemoigne/psfweb/Thessaloniki.htm

Physique-Sans-Frontières (PSF) PHYSICS WITHOUT BORDERS http://www.P-S-F.org E-mail : PSF1@compuserve.com FOUR SEAS CONFERENCE THIRD SESSION 16-21 APRIL - THESSALONIKI 2002 Sponsored by UNESCO-ROSTE (Venezia) Ministère des Affaires Etrangères (Paris) DAPNIA-CEA (Saclay) DESY (Hamburg) Thessaloniki - Diakonia Convention Centre 65 Nik. Plastira Street, Thessaloniki, Greece First Bulletin (updated 01/31/02) After Trieste in 1995 and Sarajevo in 1998, the third session of the "FOUR SEAS CONFERENCES" will take place in Thessaloniki (Greece) from April 16 to April 21, 2002. During this week, students from diverse origins (from every country of South-Eastern Europe, but also from the rest of the world) will hear about the most recent developments in sciences and technologies. Topics addressed are : i-) particle physics, ii-) astrophysics and cosmology, iii-) instrumentation with application to medical physics. -1- Motivation Since seven years, the "Four Seas Conferences" are a way to express the solidarity of the scientific community with all those who, under difficult conditions, seek to keep alive the diverse intellectual and cultural links that constitute the essence of our civilisation. Our efforts are oriented towards

24. Friends Of Scotland - Features - Education - What Caused The Ripple In The Micro but it also marks the beginning of another exciting chapter for astrophysics asit grappling with questions like what is the nature of dark matter (the stuff http://www.friendsofscotland.gov.uk/education/astrophysics.html

7 April 2003 BST October 2002 What caused the ripple in the Microwave Background? The Microwave Background? 21st century muzak? Hardly. Rather, the state of the universe before any galaxies were formed. Over 14 billion years ago. And whereas astronomers may once have been seeking the ‘music of the spheres’ they’re now seeking its composition. With the help of infra-red telescope instruments made in Edinburgh. The retreat from light pollution Now when astronomers and astro-physicists want to gaze at the stars they have to go to mountain tops that meet an exacting brief. Not only do they have to be high enough to minimise light pollution and increase the chances of cloudless nights and dry air, they also have to be close to the ocean to benefit from the planet’s purest and most smoothly flowing air. Only school parties and guests at the Royal Observatory’s Visitor Centre stargaze from Blackford Hill these days, or rather, these nights. For the cutting-edge professors of Edinburgh University’s Institute for Astronomy who are based at Blackford Hill, real-time observation requires trips to those faraway mountain tops in places like Hawaii and Chile. But it’s no doubt pleasing to know that crucial high-tech components for many of the telescopes they use half way across the world were made in the labs of their neighbours at the

25. Tim Connors - Project Information be for stuff that is not going to be published; It could be conference proceedings;it could be cutting edge astrophysics. Non-Baryonic dark matter Searches. http://astronomy.swin.edu.au/~tconnors/sao-projects/

Tim Connors - Project information This page contains information for all SAO students submitting project and and to me. Come back as necessary, I may have added or corrected links since last time you came. Please feel free to email me at if you have any questions on project assessment, or on the Projects listed below. Also, mail me if you come across a broken link in this page. And, by all means, mail me if you find some better links! However, all questions about computers, CD-ROMs, Internet access, etc. should go to SAO helpdesk and ltshelp For any work submitted to me please make sure you include 1) Your Name 2) SAO Student number 3) Unit (eg. HET603B, HET604, etc) and Semester (ie. S1, 2003) 4) Title of Work. Work should be submitted as (in order of preference - given that I am using UNIX here) OpenOffice documents, Word documents (ick), or PDF documents (although the latter doesn't allow me to modify the file and return it to you). Assessment Details Before reading any further please carefully read SAO Assessment Details (in fact, read that whole page) if you haven't done so. Also, the sample essay on that page shows you how to lay out your references.

26. Wheeling Jesuit University energy astrophysics.” This field deals with the X-ray, gamma-ray and cosmic rayuniverse; and covers topics such as black holes, quasars and dark matter. http://www.wju.edu/about/adm_news_story.asp?iNewsID=710&strBack=/about/adm_news.

27. E-Preprints Astro-ph/9411 At DESY 9411038 From griest@astrophys.UCSD.EDU (Kim Griest) Date Wed, 9 Nov 94 112733PST (25kb) Title THE PARTICLE AND astro-physics OF dark matter Author Kim http://www-library.desy.de/preparch/astro-ph/9411/00index.html

E-Preprints astro-ph/9411 at DESY The complete Postscript Version of this paper is also available locally. However to conserve disk space this version might be "staged" to tape. Access the local version of astro-ph/9411013. N.B. You can find the full abstact of astro-ph/9411013 at the Los Alamos Preprint server. The complete Postscript Version of this paper is also available locally. However to conserve disk space this version might be "staged" to tape. Access the local version of astro-ph/9411020. N.B. You can find the full abstact of astro-ph/9411020 at the Los Alamos Preprint server. The complete Postscript Version of this paper is also available locally. However to conserve disk space this version might be "staged" to tape. Access the local version of astro-ph/9411038. N.B. You can find the full abstact of astro-ph/9411038 at the Los Alamos Preprint server. Paper: astro-ph/9411047 From: masperi_luis The complete Postscript Version of this paper is also available locally. However to conserve disk space this version might be "staged" to tape. Access the local version of astro-ph/9411047.

28. UNM - Quantum Spring 1998 - Unmasking Secrets Of The Universe This is really important for particle physics, cosmology and astrophysics, Yves Declais, now One of the best candidates for the dark matter, for the http://www.unm.edu/~quantum/quantum_sp1998/nutrino.html

Unmasking the Secrets of the Universe UNM TEAM STUDIES THE ELUSIVE, ENIGMATIC NEUTRINO By Denise Tessier False FACTS are highly injurious to the progress of science, for they often endure long; but false VIEWS, if supported by some evidence, do little harm, for everyone takes a salutary pleasure in proving their falseness; and when this is done, one path toward errors is closed and the road to truth is often at the same time opened." Charles Darwin, 1809-1882 C osmologists, physicists and astronomers generally hold this view: that 10 billion to 20 billion years ago the universe had no size, was infinitely hot, and suddenly exploded in the "Big Bang," creating the universe as we know it. In the nuclear fusion reactions that followed this singular event, mysterious particles were created and scattered, swarming into clusters that exerted enough pull on ordinary matter to create stars. These clusters are known as "dark matter." But scientists are not sure what dark matter is. Dark matter cannot be seen and is detected only indirectly when celestial neighbors react to its presence in nearly imperceptible ways. One view is that dark matter could be comprised of neutrinos. Neutrinos are particles theorized in the 1930s and first discovered in the 1950s as a by-product of nuclear reactors and atomic bombs.

29. First Gamma Rays Associated With Galaxy Clusters are accelerated by shocks or produced in the annihilation of dark matter particles)might from galaxy clusters led to a new era in astrophysics and cosmology. http://universe.gsfc.nasa.gov/press/2001/cw01_08.html

First Gamma Rays Associated With Galaxy Clusters Contact: Christopher Wanjek wanjek@gsfc.nasa.gov April 5, 2001 Greenbelt, Md. Clusters of galaxies, the largest bound structures in the universe, may admit gamma rays, a discovery that would have broad implications for the structure, evolution and mass content of the universe. Dr. Sergio Colafrancesco of the Astronomical Observatory of Rome has found a probable association between known galaxy clusters and unidentified gamma-ray sources that have stymied astronomers for several years. He presents his findings today at the Gamma Ray 2001 conference in Baltimore, Maryland. "If these gamma-rays are truly associated with galaxy clusters, they could be produced by cosmic-ray collisions in the intergalactic space, by the annihilation of dark matter particles inhabiting the clusters, or by unknown active galaxies, among other possibilities," said Colafrancesco. "Yet any of these possibilities would be of particular interest to the scientific community." Gamma rays represent the most energetic form of radiation. These high-energy photons are produced in cataclysmic events, such as the flow of extremely hot gas towards a black hole or the collision of elementary particles moving at nearly the speed of light.

30. Dark Matter - Examining The Evidence From Lensing A PSR Resource. Introduction to Astrophysics. Cosmic Hide and Seek the Search for the Missing Mass by Chris Miller Copyright © 1995 by Chris Miller, all rights reserved. searching for the elusive dark matterthe other 90% of the universe. dark matter. What do scientists look for when they search for dark matter? We cannot see http://www.astro.rug.nl/~onderwys/sterIIproject98/louise

How strong is the evidence provided by gravitational lensing for the existence of dark matter? by Steven O. Louise Abell 2218 - A much studied example of weak and strong lensing by a cluster of galaxies (Shown here: an HST image of the core of the cluster) Table of contents: Abstract 1. Introduction 1.1 What is gravitational lensing? 1.2 Weak and strong lensing ... Appendix A. Other methods for determining dark matter mass Abstract MOND would seem to be a viable alternative to dark matter. 1. Introduction Gravitational lensing provides some of the strongest evidence in support of dark matter. Since our aim is to examine the strength of all such evidence, studying the strength of the evidence from lensing is an integral part of our investigation. One of the greatest advantages of gravitational lensing is that, unlike the virial , and X-raymethod s, the mass can be determined independent of the dynamical state of the cluster, and in a more direct way. If this method is proven to be sufficiently reliable in its application to clusters of galaxies, the evidence for dark matter will be greatly strengthened. The questions I have set myself to answer are: how strong is the evidence from lensing for the existence of dark matter? And can wrong assumptions explain the mass discrepancy?

31. Astro Physics regarding the theory of 'dark matter' had not only been taught 'how' to manipulate dark matter to achieve certain ends, MACHO's in the dark matter theory is not hard http://www.ancient-astronaut.com/astro-why.htm

Why Astrophysics? [Please read the basic background document before proceeding; entitled Astrophysics Astrophysics could easily be the most significant way of proving the ancient astronaut theory. If it could be proved that information regarding the theory of 'Dark Matter' had not only been passed on to the ancient civilisations of the world but also these same ancient civilisation had been taught 'how' to manipulate dark matter to achieve certain ends, then history would certainly need to be re-written. We believe it maybe time to re-examine ancient devices, beliefs and constructions, to establish whether this hypothesis could be true. Throughout history mythologies have discussed a unifying force that binds the Universe, Plato and the esoteric Vril-ya organisation (to name only two) have postulated this idea, later this force was given an identity and eventually was consumed by the illusion of God. But what if the ancients were alluding to an advanced knowledge that they did not understand? As with genetics, DNA and flying machines, were the ancients trying as best they could, to relay this information that had been given to them by the Anunnaki? The theory of WIMPS and MACHO's in the dark matter theory is not hard to grasp but impossible to explain without the complexities and technicalities of our modern languages. How do you explain sub-atomic particles that make up 90-99% of the matter in the universe to a 4 year old child?

32. HVORFOR DARK MATTER? Mørkt Stof i Universet Hvilke muligheder er der og hvilke er sandsynlige Anne Dederichs Thorbjørn List Jeppsson Hvorfor dark matter? udsender nogle form for stråling dark matter eller mørk stof. Teorien om dark matter kunne være "the missing link" mellem Hvad er dark matter? dark matter (DM) strækker sig fra http://www.tac.dk/~list/research/darkmatter

i Kosmologi Hvilke muligheder er der og hvilke er sandsynlige... Skrevet af Indholdsfortegnelse Indholdsfortegnelse Hvorfor Dark Matter? Hvad er Dark Matter? Teori 1: Baryonisk stof ... Referencer Hvorfor Dark Matter? A B (M A /L A B /L B Teorien om Dark Matter kunne være "the missing link" mellem teorierne, der beskriver det homogene glatte Univers i sine unge år, og det klumpede Univers, vi befinder os i for tiden. Hvad er Dark Matter? eV = 10 M) til tunge sorte huller (10 skal Teori 1: Baryonisk stof Teori 2: Ikke-baryonisk stof Neutrinoer cm Hvis Vi kender mindst 4 slags neutrinoer: elektronneutrino + antineutrino nuonneutrino + antineutrino I volumen V er der partikler, hvor p Virialteoremet hvor er den gennemsnitlige dispersionshastighed af de objekter, der binder systemet (gravitioner). denne ligning giver sammen med at cold varm baryonic Hot Dark Matter (HDM) M Warm Dark Matter (WDM) WDM har en hvilemasse af 1 keV. WDM var relativistisk indtil mc kT = mc Cold Dark Matter (CDM) Axioner Axioner er de mindste CDM-elementer med en masse af 10 a eV, vil

33. Nuclear And Astro Physics In Underground Laboratory@ Nuclear and astro physics in underground laboratory Program International Institutefor Advanced 1440, dark matter search and study of double beta decay by http://www.iias.or.jp/event/ndm-p02.html

Nuclear and astro physics in underground laboratory Program International Institute for Advanced studies (IIAS) Feb.23, 2002 Low temperature gravitational wave telescope ICRR Tokyo Univ. K.Kuroda Gravitational moment of elementary particles and their measurement Kobe Tokiwa College M.Tanaka High sensitive measurement of impurities JAERI Tokai M.Oshima Atmospheric radon and precipitation rates International Christian University H.B.Greenfield Lunch MOON for Double Beta Decays, Solar Neutrinos and S upernova Neutrinos IIAS, Spring-8 H.Ejiri Search for neutrinoless double beta decay with DCBA KEK N.Ishihara Double Gamow Teller excitations and double beta decay RCNP Osaka Univ. K.Takahisa Coffee Dark matter search and study of double beta decay by ELEGANT VI Dept. Phys. Osaka Univ. I.Ogawa

34. Physics Department Profiles Particle Astrophysics and Condensed matter Physics. Professor of Physics. in search of dark matter in the form of Theoretical Condensed matter Physics. Professor of Physics. http://www.stanford.edu/group/physics/profile.html

Physics Department Profiles A brief outline is given below of the research interest of each of the research groups in the Physics Department. The Stanford graduate school is characterized by a highly flexible approach to graduate education. Graduate students in Physics are allowed to pursue their studies with faculty members in other Departments such as Applied Physics, Chemistry, Electrical Engineering,and the Stanford Linear Accelerator Center. The brochures for these groups should be reviewed to get a full view of the current research at Stanford. Some of these will be included in the admission package sent out containing information on our Department. If you need further information, please write directly to the faculty, c/o Department of Physics. Patricia Burchat Blas Cabrera Steven Chu Savas Dimopoulos ... Shoucheng Zhang Patricia Burchat, Associate Professor Experimental Particle Physics Associate Professor of Physics, B. Appl. Sci. Eng., 1981, University of Toronto; Ph.D., 1986 Stanford University; Postdoctoral Fellow, Santa Cruz Institute for Particle Physics, 1986-88; Associate Professor, University of California, Santa Cruz, 1988-92; Associate Professor, University of California, Santa Cruz, 1992-94; Associate Professor, Stanford University 1995-present; National Science Foundation Presidential Young Investigator Award, 1991. Research efforts in experimental particle physics are focussed on heavy quark decays. Production and decay properties of the charm quark are currently being studied with data collected by the E791 collaboration in a fixed-target hadroproduction experiment at the Fermi National Accelerator Laboratory, with an emphasis on D-meson mixing and semileptonic decays. A new detector is being developed for studies of violation of charge-parity symmetry in decays of mesons containing the bottom quark, at the Asymmetric B Factory at the Stanford Linear Accelerator Center.

35. Puplications Phys. B632 (2002) 363 hepph/0201287. 21) Interacting dark matter disguisedas Warm dark matter C. Boehm, A. Riazuelo, SH Hansen, R.Schaeffer Phys. Rev. http://www-astro.physics.ox.ac.uk/~hansen/papers/papers.html

Publications Papers "The origin of cores and density profiles of baryonic structures" S. H. Hansen, J. Stadel Subm. to ApJ [astro-ph/0303416] "Extraction of cluster parameters with future Sunyaev-Zel'dovich observations" N. Aghanim, S. H. Hansen, S. Pastor, D. Semikoz Subm. to JCAP [astro-ph/0212392] "Observational constraint on the fourth derivative of the inflaton potential" C. Caprini,S. H. Hansen, M. Kunz MNRAS (2003) 212 [hep-ph/0210095]. "The impack of relativistic corrections and component separation in the measurement of the SZ effect and on the small angular scale non-Gaussianity of the CMB" J. M. Diego, S. H. Hansen, J. Silk MNRAS (2003) 796 [astro-ph/0207178] "First measurement of cluster temperature using the thermal Sunyaev-Zeldovich effect" S.H. Hansen, S. Pastor, D.V. Semikoz Astrophys. J. (2002) L69 [astro-ph/0205295] "Cosmological bounds on neutrino degeneracy improved by flavor oscillations" A.D. Dolgov, S.H. Hansen, S. Pastor, S.T. Petcov, G.G. Raffelt, D.V. Semikoz Nucl. Phys. (2002) 363 [hep-ph/0201287] "Interacting Dark Matter disguised as Warm Dark Matter" C. Boehm, A. Riazuelo, S. H. Hansen, R.Schaeffer

36. Spectrum Of Physics - A Physics Directory: Special Relativity, Quantum Theory, E abs/astroph/9706129; The Particle- and astro-physics of dark Matterhttp//xxx.lanl.gov/abs/astro-ph/9411038; The Physics of Microwave http://www.tardyon.de/links/cosmo/reviews astro.html

Luxon Theory Time Theory copenhagen experiment SPECTRUM OF PHYSICS root top A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation http://xxx.lanl.gov/abs/astro-ph/0004404 Advanced Statistical Methods for Large-Scale Structure Studies http://xxx.lanl.gov/abs/astro-ph/9510035 Ages of Globular Clusters from Hipparcos Parallaxes of Local Subdwarfs http://xxx.lanl.gov/abs/astro-ph/9704150 Baryonic fraction in the cold plus hot dark matter universe http://xxx.lanl.gov/abs/astro-ph/9710078 Big-bang Nucleosynthesis Enters the Precision Era http://xxx.lanl.gov/abs/astro-ph/9706069 Calculation of Cosmic Background Radiation Anisotropies and Implications http://xxx.lanl.gov/abs/astro-ph/9607088 Characterizing the Peak in the CMB Angular Power Spectrum http://xxx.lanl.gov/abs/astro-ph/0002162 Classical and Quantum Theory of Perturbations in Inflationary Universe Models http://xxx.lanl.gov/abs/astro-ph/9307016 Cluster Winds Blow along Supercluster Axes http://xxx.lanl.gov/abs/astro-ph/9808018 CMB Anisotropies and the Determination of Cosmological Parameters http://xxx.lanl.gov/abs/astro-ph/0002249

37. Links To Dark Matter And Particle Astrophysics Sites Baryonic dark matter EROS; POINTAGAPE; MACHO; MOA; OGLE. Particle physics CERN;DESY; RAL; FNAL; SLAC; BNL; Particle Data Group; Particle/Astro Physics e-Print Archive; http://www.shef.ac.uk/~phys/research/pa/links.html

Links to Dark Matter and Particle Astrophysics Sites Cosmology and dark Matter: MAXIMA Cosmic Microwave Background Survey BOOMERanG Cosmic Microwave Background Survey Supernova Cosmology Project High-Z Supernova Search ... SNAP Next Generation Supernovae Survey Non-baryonic dark matter: Direct WIMP Searches: UKDMC CDMS Ge/Si Bolometer EDELWEISS Ge Bolometer DAMA NaI Scintillator ... Interactive WIMP Dark Matter Limit Plotter Axion Searches: PVLAS CAST ADMX Double Beta Decay Experiments: Heidelberg-Moscow Ge Gotthard Xe TPC NEMO Mo TPC EXO Xe TPC ... MAJORANA Ge Baryonic dark matter: EROS POINT-AGAPE MACHO MOA ... OGLE Other Underground Laboratories and Experiments: Gran Sasso Modane Canfranc Kamioka ... MINOS (Soudan) Indirect WIMP Searches: ANTARES AMANDA NESTOR NEMO ... HESS Particle physics: CERN DESY RAL FNAL ... HEP-DATA Astrophysics: HST ING AAO ESO ... HOME

38. Astrophysics: Oxford University Graduate Studies Prospectus holes, dark matter and largescale structure. Further details of current researchin astrophysics may be found by consulting the website www-astro.physics.ox.ac http://www.admin.ox.ac.uk/gsp/courses/mathsphys/astr.shtml

Search Graduate Prospectus Download application material Graduate Admissions Office International Office ... Additional subject information Astrophysics Graduate Studies Prospectus Courses Research in Astrophysics at Oxford spans a wide range of topics - from theoretical studies of the formation of structure in the Universe to high-precision observations of stars. Astronomers at Oxford are making fundamental contributions to observational and theoretical cosmology, and the astrophysics of stars, galaxies, black holes, dark matter and large-scale structure. Further details of current research in astrophysics may be found by consulting the website www-astro.physics.ox.ac.uk Astronomers at Oxford are also studying distant clusters of galaxies, quasars, radio galaxies and galactic star-forming regions. On the theoretical side, work is in progress on the evolution of single and binary stars, supernovae, gamma-ray bursts, the structure of compact objects, galaxy formation, the cosmic microwave background, and identification of the experimental signatures of dark matter. Much of the observational work is undertaken using PPARC-supported telescopes, e.g. the UK Infrared Telescope and the James Clerk Maxwell mm-wave Telescope in Hawaii, the William Herschel Telescope in the Canary Islands, the Anglo-Australian Telescope, the Gemini Telescopes in Hawaii and Chile, the UK-based MERLIN radio synthesis array, and the numerous facilities of the European Southern Observatory in Chile. Oxford astronomers also use non-UK facilities, e.g. the Very Large Array in New Mexico and the Subaru 8-m telescope in Hawaii, and space facilities such as the Hubble Space Telescope, and the Chandra X-ray Observatory. The UK Project Scientist for the Gemini Project is based in the sub-department. Astronomical instrumentation to be used on the Subaru and ESO telescopes is being designed and constructed in the sub-department. There are about 70 astrophysicists engaged in research in Oxford (most in Astrophysics, others in

39. Home Page Von Wolfgang Priester the Universe and dark matter Clues from the Lymanalpha Forest by Carsten vande Bruck and Wolfgang Priester in dark matter in Astro- physics and Particle http://www.astro.uni-bonn.de/~priester/

Prof. em. Dr. Wolfgang Priester D-53121 Bonn / GERMANY E-Mail: priester@astro.uni-bonn.de Phone: +49-228-73-3782 Fax: +49-228-73-3672 Zur IAEF Home Page Main fields of research Astrophysics Cosmology Radioastronomy Upper Atmosphere Physics IAEF was founded by Bonn University in 1964 under its director Prof. Wolfgang Priester (1964-1989). His curriculum vitae can be found in "Who's Who in the World" and in ""Wer ist Wer", "Das Deutsche Who's Who"". When he became emeritus professor in August 1989 his research interest concentrated on cosmology: Is our permanently expanding universe a closed space with spherical metric? This is the result of the BONN-POTSDAM-model (BN-P-model), derived by Friedmann-regression-analysis from 1260 Lyman-alpha absorption lines in the spectra of 21 quasars with redshifts between 1.8 and 4.4. (J. Hoell, D.E. Liebscher, W. Priester 1992, 1994; see Confirmation of the Friedmann-Lemaitre Universe, Astron. Nachr. 315, 89-96 (1994). The analysis is based on the assumption that the spongelike bubble structure in the distribution of galaxies expands essentially with the Hubble expansion whereas internal evolution of the distribution is of minor importance. The sum of the density parameter plus the Lambda parameter is 1.094. This number corresponds to a present curvature radius of the ever expanding closed universe of 36 Giga- lightyears. For details we refer to our paper: "The Cosmological Constant, the Age of the Universe and Dark Matter: Clues from the Lyman-alpha Forest" by Carsten van de Bruck and Wolfgang Priester in "Dark Matter in Astro- physics and Particle Physics 1998" (ed. H.V. Klapdor- Kleingrothaus and L. Baudis) p. 181-196, Inst. of Physics Publishing, Bristol and Philadephia 1999. It can also be obtained from http://xxx.lanl.gov astro-ph/9810340 21 Oct 1998.

40. EDUMAP EDU2 PHYSICS MODERN; ACCELERATOR; ASTRO PHYSICS; - ASTROPHYSICS TITLE; ATOMICPARTICLE; TITLE; BLACK HOLE; CONSTELLATION; COSMIC RADIATION; dark matter; DEEP SKY; http://www.my-edu2.com/cgi-local/crtmap.cgi?physic4.htm

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