Auger Line Shapes in Solids

Total Page:16

File Type:pdf, Size:1020Kb

Auger Line Shapes in Solids Auger Line Shapes in Solids Pierre Victor Auger (1899-1993) who discovered the law of the Auger effect in 1925 who discovered the Auger effect in 1923 1 Core-levels observed in photoemission are resonances and width is large for high binding energies Core-levels observed in photoemission are resonances and width is large for high binding energies Fe1s binding energy=7112 eV Width > 5 eV Decay mechanisms: X-ray emission, Auger electron emission. Auger electrons are seen by the ESCA apparatus along with photoelectrons. Their energies are independent of the photon energy. X− ray notation level Ks1 1/2 Ls1 2 1/2 Lp2 2 1/2 Lp3 2 3/2 Ms1 3 1/2 Mp2 3 1/2 Mp3 3 3/2 Md4 3 3/2 Md5 3 5/2 Ns1 4 1/2 Np2 4 1/2 Np3 4 3/2 Nd4 4 1/2 Nd5 4 3/2 Nf6 4 5/2 Nf7 4 7/2 Meitner-Auger Effect and Spectroscopy An important spectroscopy is based on the Auger Effect. Actually, this effect was first reported in 1923 in Zeitschrift für Physik by the Austrian Physicist Lise Meitner (1878-1968). In 1925, the great French physicist Pierre Auger (1899- 1993) rediscovered the effect while investigating in a bubble chamber the emission of an electron from an atom that absorbs a X-ray photon, that is, photoemission. The photoelectrons have kinetic energy Ek = hν − EB, where EB is one of the binding energies of the atom inner levels. However the Auger electrons have ν-indepedent energies given approximately by the empirical Auger law. B BB EAuger (αβγ )=E ( α ) - E ( β ) -E ( γ ) 7 B BB EAuger (αβγ )=E ( α ) - E ( β ) -E ( γ ) Pierre Victor Auger (1899-1993) X-rays of adequate energy produce a primary hole in the state α of binding energy of EB(α) and a photoelectron; since the ion with a core hole is unstable, the primary holes is filled up by an electron in a less bound level β, and the energy gained in the process is taken by an electron in level γ, than is emitted as the Auger electron. For particular transition to happen, it is necessary that the primary hole is deep enough (its binding energy must exceed the sum of those of β and χ). γ γ β β α α 8 The Auger transitions are denoted by the spectroscopic symbols of the shells (or, more precisely, sub-shells) involved: thus a KL1M2 transition is due to a primary hole in the K shell that decays leaving in the final state L1 and M2 holes and an Auger electron. Μ2 L1 Κ One speaks about Core-Core-Core, Core-Valence-Valence, etc.,transitions depending on the levels that are involved. The Auger effect is caused by the Coulomb interaction: two electrons of the system collide and while one fills up the primary hole, the other is shot out as the Auger electron. The energy of the primary-hole state is shared between the Auger electron and the ion left behind. 9 AES=Auger Electron Spectrum of Cd vapor (Z=48) X− ray notation level Ks1 1/2 M4 initial hole Ls1 2 1/2 Lp2 2 1/2 N4,5 final Lp3 2 3/2 holes Ms1 3 1/2 Mp2 3 1/2 Mp3 3 3/2 Md4 3 3/2 Md5 3 5/2 Ns1 4 1/2 Np2 4 1/2 Np3 4 3/2 Nd4 4 1/2 Nd5 4 3/2 Nf6 4 5/2 Nf7 4 7/2 11 KL11 M Auger transition in the simplest electron picture: L11+→ M Kk +the other electrons are (approximately) spectators 12 KL11 M Auger transition in the hole picture is simplest: Kk+→ L11 + M hole k is in continuum 13 X decay is faster when the involved levels are distant in energy, because of the ν3 factor in the transition probability due to the density of photon final states. The Auger decay prevails if the states α, β and γ are near in energy Auger is the dominant for inner shell holes of light atoms, while in heavy ones X decay is much more likely Wentzel (1927 ) theory: αβγ transition Primary holes final holes Primary holes: deep level α and free state k final holes : the spin-orbitals β and γ γ β α Two-step model: the photoemission process produces ion in its meta-stable ground state- Deep hole creation and Auger decay are disjoint processes . 15 Wentzel (1927 ) theory: αβγ transition Mechanism: the smoking gun The Auger transition is a Coulomb collision between two holes and is an energy conserving process. (in reality the other electrons are also involved in some way) In the hole picture, the initial state |Φi > and the final state |Φf > of the atom are represented by 2 × 2 Slater determinants; they have the same energy and are coupled by the Coulomb interaction. In a KLM transition, |Φi >=Det|ψ1sψk| --> |Φf >=Det|ψ2sψ3s| 2π 2 Rate by Fermi golden rule PHif =ΦΦ| i C f | . 16 An alternative mechanism : internal photoemission Μ Μ2 2 hν L L1 1 Κ Κ One of electrons in the upper states β, γ could fill up the deep hole via a normal radiative process, emitting a X-ray photon; this photon could then cause the photoemission of the other electron. Would’nt the final state be the same? Indeed, this alternative process does exist, and has the name of internal photoemission; unlike the Auger effect, it obeys optical selection rules. The transition probability of the internal photoemission can be calculated by perturbation theory, but since it is a second-order process in A.P it turns out to be quite small compared to the Auger effect. 17 Atomic Auger Selection Rules 2 Selection rules arise in the two-step model from the conservation of J , Jz and parity between the initial, core-hole state and the final state including the Auger electron. 2 2 In the L-S approximation, L , Lz and S , Sz are also conserved, while in the jj scheme, the states are labeled by the j quantum numbers. KLL transitions If the spin-orbit interaction is more important than the Coulomb interaction, the jj scheme applies. If the Coulomb interaction dominates, the LSMLMS scheme is OK. The pure jj scheme one would predict 6 transitions, namely, KL1L1,KL1L2, KL1L3,KL2L2,KL2L3, and KL3L3. L3 L 3 L3 L L 3 L3 3 L2 L 2 L2 L L 2 L2 2 L1 L 1 L1 L L 1 L1 1 K K 18 K K K K In the pure LS scheme, the 5 possible final states are: 2s22p4 3P is forbidden by 06 1 22sp→ S parity conservation; indeed, the primary hole has L=0 2 4 3 1 and is even, 2s 2p P is 15 P even and has L=1 ; by L 22sp → 3 P allowed conservation the Auger electron must be in a p state, which is odd.Hence 1S the final state is odd. 22sp24→ 3 P The transition to the odd 1 D 2s12p5 3P atomic final state is allowed, and one predicts 5 lines. LS terms split by Coulomb interaction 19 When the spin-orbit interaction is introduced, in intermediate coupling the forbidden final-state splits : 2 4 3 3 3 3 2s 2p P → P2, P1, P0; 3 then, states with the same j and different spin mix: P2 mixes with 1 3 1 2 4 D2 and P0 mixes with S0 from the same 2s 2p configuration. Now the decay can occur with d or s Auger electrons. 1 =3 + 2 41 S jPS0 from0 2s 2p mixed parity 33 24 3 P→= jP1 from even and J=1 22sp→ P 1 =3 + 2 41 1 j2 from PD22 2s 2p mixed parity D 3 P1 even and J=1 requires Auger electron in even state with J=1 − forbidden 21 1 =3 + 2 41 S jPS0 from0 2s 2p mixed parity 33 24 3 P→= jP1 from even and J=1 22sp→ P 1 =3 + 2 41 1 j2 from PD22 2s 2p mixed parity D 3 P1 even and J=1 requires Auger electron in even state with J=1 − forbidden 3 3 P2 and P0 become more and more allowed as Z grows. 3 Instead, P1 remains purely P and forbidden (as long as one can neglect the mixing with higher configurations). Thus, the number of lines grows to 9. 0 61 Allowed Auger transitions 22spS , in intermediate coupling 1 51 3 3 3 2sp 2 P20, P , P 1, P 2, 2spS2 2 41 , 3P , 3 P , 1 D 0 02 2 22 Resonant Photoemission Example: transition metal like Co, or oxides like CuO photo Photoemission with electron hνε=(3 dp ) − ε (3 ) εεk =(3dp ) − ε (3 ) vacuum level 3d band Fermi level d hole 3p core level 23 If the photon is tuned to the transition 3p 3d the Co is left with one less 3p electron and an excess 3d electron above the Fermi level. Then a two electron (Auger transition ) takes a 3d electron to 3p and a second 3d electron above the vacuum. This final state resonates with the direct 3d photoemission (Fano resonance). Core-Valence-Valence transitions in solids: Lander independent-particle theory Level scheme E ε k = kinetic energy of Auger electron ε k vacuum level ε1 =binding energyof level 1= electron jumps to free state =energyof hole in level 1 NE()=∑ δω ( − εk ) k∈ BZ Auger law: ε1 εεε= ++ ε ε ck12 2 core-hole→ 2 valence holes+Auger electrons electron jumps to core Auger spectrum: ε−+ εε ε εC ck(12 )= Auger energy 27 CVV transitions in solids: Lander theory (1953) Level scheme εck−+( εε12 )= εAuger electron energy E All hole pairs such that εε12+= ω ε k ε= εω − vacuum level contribute to spectrum at kc.
Recommended publications
  • Sterns Lebensdaten Und Chronologie Seines Wirkens
    Sterns Lebensdaten und Chronologie seines Wirkens Diese Chronologie von Otto Sterns Wirken basiert auf folgenden Quellen: 1. Otto Sterns selbst verfassten Lebensläufen, 2. Sterns Briefen und Sterns Publikationen, 3. Sterns Reisepässen 4. Sterns Züricher Interview 1961 5. Dokumenten der Hochschularchive (17.2.1888 bis 17.8.1969) 1888 Geb. 17.2.1888 als Otto Stern in Sohrau/Oberschlesien In allen Lebensläufen und Dokumenten findet man immer nur den VornamenOt- to. Im polizeilichen Führungszeugnis ausgestellt am 12.7.1912 vom königlichen Polizeipräsidium Abt. IV in Breslau wird bei Stern ebenfalls nur der Vorname Otto erwähnt. Nur im Emeritierungsdokument des Carnegie Institutes of Tech- nology wird ein zweiter Vorname Otto M. Stern erwähnt. Vater: Mühlenbesitzer Oskar Stern (*1850–1919) und Mutter Eugenie Stern geb. Rosenthal (*1863–1907) Nach Angabe von Diana Templeton-Killan, der Enkeltochter von Berta Kamm und somit Großnichte von Otto Stern (E-Mail vom 3.12.2015 an Horst Schmidt- Böcking) war Ottos Großvater Abraham Stern. Abraham hatte 5 Kinder mit seiner ersten Frau Nanni Freund. Nanni starb kurz nach der Geburt des fünften Kindes. Bald danach heiratete Abraham Berta Ben- der, mit der er 6 weitere Kinder hatte. Ottos Vater Oskar war das dritte Kind von Berta. Abraham und Nannis erstes Kind war Heinrich Stern (1833–1908). Heinrich hatte 4 Kinder. Das erste Kind war Richard Stern (1865–1911), der Toni Asch © Springer-Verlag GmbH Deutschland 2018 325 H. Schmidt-Böcking, A. Templeton, W. Trageser (Hrsg.), Otto Sterns gesammelte Briefe – Band 1, https://doi.org/10.1007/978-3-662-55735-8 326 Sterns Lebensdaten und Chronologie seines Wirkens heiratete.
    [Show full text]
  • Physiker-Entdeckungen Und Erdzeiten Hans Ulrich Stalder 31.1.2019
    Physiker-Entdeckungen und Erdzeiten Hans Ulrich Stalder 31.1.2019 Haftungsausschluss / Disclaimer / Hyperlinks Für fehlerhafte Angaben und deren Folgen kann weder eine juristische Verantwortung noch irgendeine Haftung übernommen werden. Änderungen vorbehalten. Ich distanziere mich hiermit ausdrücklich von allen Inhalten aller verlinkten Seiten und mache mir diese Inhalte nicht zu eigen. Erdzeiten Erdzeit beginnt vor x-Millionen Jahren Quartär 2,588 Neogen 23,03 (erste Menschen vor zirka 4 Millionen Jahren) Paläogen 66 Kreide 145 (Dinosaurier) Jura 201,3 Trias 252,2 Perm 298,9 Karbon 358,9 Devon 419,2 Silur 443,4 Ordovizium 485,4 Kambrium 541 Ediacarium 635 Cryogenium 850 Tonium 1000 Stenium 1200 Ectasium 1400 Calymmium 1600 Statherium 1800 Orosirium 2050 Rhyacium 2300 Siderium 2500 Physiker Entdeckungen Jahr 0800 v. Chr.: Den Babyloniern sind Sonnenfinsterniszyklen mit der Sarosperiode (rund 18 Jahre) bekannt. Jahr 0580 v. Chr.: Die Erde wird nach einer Theorie von Anaximander als Kugel beschrieben. Jahr 0550 v. Chr.: Die Entdeckung von ganzzahligen Frequenzverhältnissen bei konsonanten Klängen (Pythagoras in der Schmiede) führt zur ersten überlieferten und zutreffenden quantitativen Beschreibung eines physikalischen Sachverhalts. © Hans Ulrich Stalder, Switzerland Jahr 0500 v. Chr.: Demokrit postuliert, dass die Natur aus Atomen zusammengesetzt sei. Jahr 0450 v. Chr.: Vier-Elemente-Lehre von Empedokles. Jahr 0300 v. Chr.: Euklid begründet anhand der Reflexion die geometrische Optik. Jahr 0265 v. Chr.: Zum ersten Mal wird die Theorie des Heliozentrischen Weltbildes mit geometrischen Berechnungen von Aristarchos von Samos belegt. Jahr 0250 v. Chr.: Archimedes entdeckt das Hebelgesetz und die statische Auftriebskraft in Flüssigkeiten, Archimedisches Prinzip. Jahr 0240 v. Chr.: Eratosthenes bestimmt den Erdumfang mit einer Gradmessung zwischen Alexandria und Syene.
    [Show full text]
  • UNESCO – Kalinga Prize Winner – 1971 Pierre Victor Auger a Life in the Service of Science
    Glossary on Kalinga Prize Laureates UNESCO – Kalinga Prize Winner – 1971 Pierre Victor Auger A Life in the Service of Science French Physicist, Discoverer of the Atomic Auger Electronic Effect. [Born : Paris 14th May, 1899 Died : Paris 25th December 1993] Professor Auger’s outstanding professional career covered Physics, Nuclear Power & Space Research, Organization and Administration of Research, Diplomatic Services & Pedagogics but also extended in to Modern Biology, Humanistic Sciences, Poetry & Arts. He was awarded with the most Prestigious Gaede – Langmuir Award “For establishing the Fundamental Principle of Auger Spectroscopy which has led to the most widely used surface analysis technique of importance to all aspects of Vacuum Science & Technology”. Energy with the Earth Atmosphere can be considered like discoverer of gigantic particle rains generated by the interaction of cosmic rays of Extreme Discharge ...Pierre Auger 1 Glossary on Kalinga Prize Laureates Pierre Victor Auger Pierre Victor Auger (May 14, 1899 – December 25, 1993) was a French Physicist, born in Paris. He worked in the fields of atomic physics, nuclear physics and cosmic ray physics. The Auger process where Auger electrons are emitted from atoms was named after him, despite the fact that Lise Meitner discovered the process a few years before in 1923. In his work with cosmic rays, he found that the cosmic radiation events were coincident in time meaning that they were associated with a single event, an air shower. He estimated that the energy of the incoming particle that creates large air showers must be at least 1015eV (electron-volts) = 106 particles of 108eV (critical energy in air) and a factor of ten for energy loss from traversing the atmosphere (Auger et al., 1939).
    [Show full text]
  • Measurements of the Maximum Depth of Air Shower Profiles at LHC Energies with the High-Elevation Auger Telescopes
    Measurements of the maximum depth of air shower profiles at LHC energies with the High-Elevation Auger Telescopes Zur Erlangung des akademischen Grades eines Doktors der Naturwissenschaften an der Fakultät für Physik des Karlsruher Instituts für Technologie (KIT) genehmigte Dissertation von Dipl.-Phys. Alaa Metwaly Kuotb Awad aus El Fayoum/Egypt Tag der mündlichen Prüfung: 21.12.2018 Referent: Prof. Dr. Dr. h.c. Johannes Blümer Korreferent: Prof. Dr. Ralph Engel Betreuer: Dr. Ralf Ulrich ii Abstract More than 100 years after their discovery, the nature of cosmic rays is still a mystery in many aspects. The subject of this thesis is to measure the mass composition of the cosmic rays at an energy range from 1015.8eV to 1017eV. This relies on the Cherenkov light emitted in the forward direction of the shower, directly pointing towards the telescopes. A new technique was proposed for the reconstruction named Profile Constrained Geometry Fit (PCGF). The benefit of this special technique is a high accuracy geometry reconstruction, which is pos- sible using only the telescope signals. A full PCGF dataset is produced for the Cherenkov dominated showers observed by the High Elevation Auger Telescopes (HEAT). The mass composition is deduced from the distribution of the maximum depth of those showers, Xmax. The first two moments of the distribution, hXmaxi, and s(Xmax), are compared to their counterparts of proton and iron simulations. The performance of the reconstruction and the analysis is studied using a complete time-dependent Monte Carlo simulation. It is a novel technique that is used for the first time in Pierre Auger, and by which the mass composition is measured in the energy region where there are signatures of cosmic ray transition from galactic to an extragalactic origin.
    [Show full text]
  • Investigating UV Nightglow Within the Framework of the JEM-EUSO Experiments
    Investigating UV nightglow within the framework of the JEM-EUSO Experiments Frej-Eric Salomon Emmoth Space Engineering, master's level 2020 Luleå University of Technology Department of Computer Science, Electrical and Space Engineering Investigating UV nightglow within the framework of the JEM-EUSO Experiments Master Thesis Space Engineering, Instrumentation and Spacecraft Author: Frej-Eric Salomon Emmoth Supervisors: Dr. Toshikazu Ebisuzaki Chief Scientist at Computational Astrophysics Laboratory, RIKEN & Dr. Marco Casolino Team Leader, EUSO Team, Research Scientist at RIKEN Examiner: Dr. Johnny Ejemalm Senior Lecturer, Lule˚aUniversity of Technology Acknowledgements I would like to first extend my most sincere gratitude to Dr. Ebisuzaki and Dr. Casolino for giving me the opportunity to do my thesis at RIKEN within the JEM-EUSO Collaboration and their invaluable help during my time there. I am also very grateful for the people at the laboratory, many of whom I today consider my friends, who made my stay in Japan so much better. I look forward to once again see the mountains of Nagano. I next want to give thanks to my family and friends for their constant support and encourage- ment. And especially to my brothers and my girlfriend who were always there to give me a push in the right direction. I am lucky to be surrounded by such great people. Lastly, I want to express my gratitude to everyone for their patience with me, with special thanks to my supervisors and my examinator in this regard. Thank you. Abstract The main mission of the JEM-EUSO (Extreme Universe Space Observatory) Collaboration is to observe Cosmic Rays.
    [Show full text]
  • Pierre Auger Et Lise Meitner
    Pierre Auger et Lise Meitner Comparaison de leurs contributions à l’effet Auger Science et société Olivier Hardouin Duparc ([email protected]) Unité mixte de Physique CNRS/CEA/X LSI, École Polytechnique, 91128 Palaiseau 4 Lorsqu’une particule incidente de forte Pour les atomes plus légers que le Lise Meitner a observé et énergie (photon X ou γ ou électron très gadolinium, il est en faveur du proces- décrit l’effet Auger quelques rapide) éjecte du cortège électronique d’un sus Auger. L’énergie du deuxième atome un électron d’une couche profonde, électron est fonction de la seule nature mois sans doute avant un électron plus externe descendra sur ce de l’atome (l’énergie de la particule Pierre Auger, en explicitant niveau ; la différence d’énergie pourra soit incidente n’intervient plus), et sa être émise en tant que rayon X, c’est de la mesure peut donc servir de moyen une suggestion des fluorescence X, soit provoquer l’éjection d’investigation spectroscopique. Britanniques Ellis d’un autre électron orbital que l’on appelle La spectroscopie Auger est utilisée électron Auger (fig. 1) [1-3]. Le rapport aussi bien à des fins de recherche fon- et Rutherford. de fréquences entre ces deux possibilités damentale que de caractérisation dans Mais sa préoccupation dépend du numéro atomique de l’atome. l’industrie. >>> était tout autre que celle de Pierre Auger et c’est donc naturellement que l’appellation ÉTAT FONDAMENTAL ÉTAT IONISÉ ÉTAT AUGER ÉTAT FINAL « effet Auger » est apparue, n = ∞ n = ∞ n = ∞ n = ∞ n = 4 n = 4 n = 4 n = 4 d’abord en Allemagne.
    [Show full text]
  • Effects of Lorentz Invariance Violation on the Ultra-High Energy Cosmic
    UNIVERSIDADE DE SÃO PAULO INSTITUTO DE FÍSICA DE SÃO CARLOS Rodrigo Guedes Lang Effects of Lorentz invariance violation on the ultra-high energy cosmic rays spectrum São Carlos 2017 Rodrigo Guedes Lang Effects of Lorentz invariance violation on the ultra-high energy cosmic rays spectrum Dissertation presented to the Graduate Pro- gram in Physics at the Instituto de Física de São Carlos, Universidade de São Paulo, to obtain the degree of Master in Science. Concentration area: Basic Physics Supervisor: Prof. Dr. Luiz Vitor de Souza Filho Corrected version (Original version available on the Program Unit) São Carlos 2017 AUTHORIZE THE REPRODUCTION AND DISSEMINATION OF TOTAL OR PARTIAL COPIES OF THIS THESIS, BY CONVENCIONAL OR ELECTRONIC MEDIA FOR STUDY OR RESEARCH PURPOSE, SINCE IT IS REFERENCED. Cataloguing data reviewed by the Library and Information Service of the IFSC, with information provided by the author Lang, Rodrigo Guedes Effects of Lorentz invariance violation on the ultra-high energy cosmic rays spectrum / Rodrigo Guedes Lang; advisor Luiz Vitor Souza Filho - reviewed version -- São Carlos 2017. 104 p. Dissertation (Master's degree - Graduate Program in Basic Physics) -- Instituto de Física de São Carlos, Universidade de São Paulo - Brasil , 2017. 1. Lorentz invariance violation. 2. Ultra-high energy cosmic rays. 3. Propagation. 4. UHECR spectrum. 5. Pierre Auger Observatory. I. Souza Filho, Luiz Vitor, advisor. II. Title. ACKNOWLEDGEMENTS Even though this work takes my name as an author, it was only possible, as everything in my life, due to several people who always supported me and, without noticing, gave me the strength to do my best.
    [Show full text]
  • Cosmic Raysrays Willwill Hithit Eacheach Ofof Youyou Duringduring Thisthis Lecturelecture What Are Cosmic Rays?
    SestoSesto Fiorentino,Fiorentino, SpringSpring--20052005 WARNINGWARNING MoreMore thanthan 100,000100,000 cosmiccosmic raysrays willwill hithit eacheach ofof youyou duringduring thisthis lecturelecture What are Cosmic Rays? Cosmic Rays (CR) are high-energy The astrophysical field of activity particles of extraterrestrial origin for particle and nuclear physics “Classical” CR are nuclei or ionized atoms ranging from a single proton up to an iron nucleus and beyond, but being mostly protons (~90%) and α particles (~9%). However the above definition is much wider and includes in fact all stable and quasistable particles: • neutrons, Secondary CR (produced by the primaries in the • antiprotons & (maybe) antinuclei, Earth’s atmosphere) consist of essentially all −12 elementary particles and nuclei (both stable and • hard gamma rays (λ < 10 cm), unstable). The most important are • electrons & positrons, • nucleons, nuclei & nucleides, • neutrinos & antineutrinos, • (hard) gammas, • esoteric particles (WIMPs, • mesons (π±,π0,K±, …, D±,…), magnetic monopoles, mini black • charged leptons (e±, µ±, τ±), holes,...). • neutrinos & antineutrinos (νe, νµ, ντ). HonorableHonorable MentionMention toto CosmicCosmic RaysRays •• OurOur planetplanet isis builtbuilt fromfrom CosmicCosmic Rays.Rays. •• CosmicCosmic RaysRays affectedaffected (and(and maybemaybe stillstill affect)affect) thethe evolutionevolution ofof thethe lifelife onon thethe EarthEarth beingbeing duringduring billionsbillions ofof yearsyears aa catalyzercatalyzer ofof mutations.mutations. ••
    [Show full text]
  • Carbon Nanomaterials in Clean Energy Hydrogen Systems - II NATO Science for Peace and Security Series
    Carbon Nanomaterials in Clean Energy Hydrogen Systems - II NATO Science for Peace and Security Series This Series presents the results of scientific meetings supported under the NATO Programme: Science for Peace and Security (SPS). The NATO SPS Programme supports meetings in the following Key Priority areas: (1) Defence Against Terrorism; (2) Countering other Threats to Security and (3) NATO, Partner and Mediterranean Dialogue Country Priorities. The types of meeting supported are generally "Advanced Study Institutes" and "Advanced Research Workshops". The NATO SPS Series collects together the results of these meetings. The meetings are co-organized by scientists from NATO countries and scientists from NATO's "Partner" or "Mediterranean Dialogue" countries. The observations and recommendations made at the meetings, as well as the contents of the volumes in the Series, reflect those of participants and contributors only; they should not necessarily be regarded as reflecting NATO views or policy. Advanced Study Institutes (ASI) are high-level tutorial courses intended to convey the latest developments in a subject to an advanced-level audience Advanced Research Workshops (ARW) are expert meetings where an intense but informal exchange of views at the frontiers of a subject aims at identifying directions for future action Following a transformation of the programme in 2006 the Series has been re-named and re-organised. Recent volumes on topics not related to security, which result from meetings supported under the programme earlier, may be found in the NATO Science Series. The Series is published by IOS Press, Amsterdam, and Springer, Dordrecht, in conjunction with the NATO Emerging Security Challenges Division.
    [Show full text]
  • Pierre Auger Observatory and KASCADE-Grande
    Pierre Auger Observatory and KASCADE-Grande Dr. Frank Morherr Pierre Victor Auger (1899-1993) • He was the discoverer of giant airshowers generated by the interaction of very high-energy cosmic rays with the earth's atmosphere . • His Fields of experimental physics were – Atomic physics (photoelectric effect); – Nuclear physics (slow neutrons); – Cosmic ray physics (atmospheric air -showers). – Made cosmic ray experiments on the Jungfraujoch • Discovery of extensive air showers (1938) • He estimated the energy to 10 15 eV • After the war, he became Director of the Department of Sciences for UNESCO. Auger Observatory Location of the auger experiment Involved 15 countries Cosmic Rays • Cosmic rays are energetic charged subatomic particles, originating from outer space. • Produce secondary particles that penetrate the Earth's atmosphere and surface. 89% of cosmic rays are protons or hydrogen nuclei 10% are helium nuclei or alpha particles 1% are heavier elements • Cosmic rays can have energies of over 10 20 eV, far higher than the 10 12 to 10 13 eV that terrestrial particle accelerators can produce • From where do they come unknown superpowerful cosmic explosion? huge black hole sucking stars to their violent deaths? From colliding galaxies? Aim of the experiment • Pierre-Auger-Observatorium worldwide greatest installation for Measurement of cosmic Rays • Surface detectors mesure the secondary particles. They detects high energy particles through their interaction with water placed in surface detector tanks • Telescope tracks the development
    [Show full text]
  • Auger: World Scientists Seek to Solve the Enigma of the Origin of Ultra High Energy Cosmic Rays
    ALICE2 Case Study Auger: World scientists seek to solve the enigma of the origin of ultra high energy cosmic rays The Auger project is an international effort to what the Cosmos’ most energetic astrophysical study the arrival on Earth of particles of the sources are and what the acceleration highest energy through measurements that mechanisms of these particles are, something determine their load and direction of arrival. that could provide information on the Universe’s According to the experts, to learn about their evolution and origin. origin would make it possible to understand With a 3,000 square kilometres covered available for international collaboration. by the Organisation of Hispanic-American area, the Pierre Auger observatory Thanks to the connectivity provided by States on 17th November 2008 (http://www. (Argentina) is the world’s largest cosmic RedCLARA for data transfer and storage, in oei.es/noticias/spip.php?article3877). rays detector. Located in the Malargüe area, 2007 the research done in the observatory in the Mendoza Province, its facilities consist determined that galaxies with active nuclei Contributing to education, the observatory of a network of 1600 detectors integrated are the most probable source of the ultra- offers guided tours around its facilities for with a set of high sensitivity telescopes; with high energy cosmic rays that get to the students and general public, and publishes them the faint ultraviolet light produced Earth; the fact was catalogued as one of 1% of the surface detector data through its by cosmic rays showers as they cross the the major achievements of that year by the website’s Events Viewer.
    [Show full text]
  • Lise Meitner (1878 – 1968)
    Lise Meitner (1878 – 1968) Lise Meitner, UNESCO lecture, March 30, 1953, Vienna www.azquotes.com/quote/573182 The master physicist and her struggle against prejudice Lars Bergström The Oskar Klein Centre, Department of Physics Stockholm University 2019-02-08 Contents: • The early years, collaboration between Lise Meitner and Otto Hahn • Physics in the early 20th century • Early achievements of Lise Meitner • The experimental discovery of nuclear fission - the surprising measurements by Otto Hahn and Fritz Strassmann, Nov. 1938 • The correct explanation – the theory of nuclear fission, Lise Meitner and Otto Frisch, Jan. 1939 • Lise Meitner in Sweden, 1938 – 1960 • Oskar Klein • Some modern knowledge about nuclei • The Nobel Prize • Summary Lars Bergström, The Oskar Klein Centre, Department of physics, 2019-02-08 2 Stockholm University The early years – being a woman in Austria-Hungary and then moving to Berlin, Germany Short biography of Lise Meitner (mostly based on ”Lise Meitner, A Life in Physics”, Univ. of California Press, 1996): • Born on November 7, 1878 (as Elise) in Vienna, to a Jewish upper-class family in Austria-Hungary, as third out of 8 children • As women were not allowed to make higher studies at public institutions, she was put in a The house in Vienna where Lise Meitner ”Bürgerschule” to study to become a teacher in French. However, as she was very talented in math was born. Photo: John Benzol and physics, she then made private studies in physics which allowed her to enroll at Vienna University. • After basic university studies with among others Ludwig Boltzmann as a very enthusiastic teacher, she worked on her PhD.
    [Show full text]