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Primordial Hydrogen-Helium Degassing, an Overlooked Major Energy Source for Internal Terrestrial Processes
HAIT Journal of Science and Engineering B, Volume 2, Issues 1-2, pp. 125-167 Copyright C 2005 Holon Academic Institute of Technology ° Primordial hydrogen-helium degassing, an overlooked major energy source for internal terrestrial processes 1, 2 Arie Gilat ∗ and Alexander Vol 1Geological Survey of Israel (ret.), 8 Yehoash St., Jerusalem 93152, Israel 2Enlightment Ltd. 33 David Pinsky St., Haifa 34454, Israel ∗Corresponding author: [email protected] Received 20 July 2004, revised 3 February 2005, accepted 16 February 2005 Abstract The currently accepted theories concerning terrestrial processes are lacking in accounting for a source of internal energy which: (a) are quickly focused, e.g. earthquakes and volcanic eruptions; (b) are of very high density; (c) provide very high velocities of energy re- lease; (d) have very high density of the energy transport and relatively small losses during transportation over long distances; (e) are quasi- constantly released and practically limitless. This energy release is always accompanied by H- and He-degassing. Solid solutions of H and He, and compounds of He with H, O, Si and metals were discovered in laboratory experiments of ultra-high PT-conditions; He-S, He-Cl, He- C, He-N structures can be deduced from their atomic structure and compositions of natural He-reach gases. Ultra-high PT-conditions ex- ist in the Earth’s interior; hence it seems most likely that some “exotic” compounds are present in the Earth’s core and mantle. During Earth’s accretion, primordial hydrogen and helium were trapped and stored in the planet interior as H- and He- solutions and compounds, stable only under ultrahigh PT-conditions that were dis- covered in recent experiments. -
Electron Bubble TPC Concept • R&D Progress • Next Steps: Towards a Cubic-Meter Prototype
Development of Cryogenic Tracking Detectors for Low- energy Solar Neutrinos Physics Seminar Southern Methodist University Monday, March 26th, 2007 Raphael Galea Columbia University/Nevis Laboratories Columbia/Nevis: J. Dodd, R. Galea, W. Willis BNL: R. Hackenburg, D. Lissauer, V. Radeka, M. Rehak, P. Rehak, J. Sondericker, P. Takacs, V. Tcherniatine Budker: A. Bondar, A. Buzulutskov, D. Pavlyuchenko, R. Snopkov, Y. Tikhonov SMU: A. Liu, R. Stroynowski Outline • Accessing the low energy solar neutrino spectrum • The Electron Bubble TPC concept • R&D progress • Next steps: towards a cubic-meter prototype R. Galea (Columbia University) SMU Physics Seminar March 26th, 2007 R. Galea (Columbia University) SMU Physics Seminar APS Study: Neutrino Matrix March 26th, 2007 Evidence of ν oscillation: • Solar Standard model provides a theory • Our understanding of neutrinos about the inner workings of the Sun. has changed in light of new • Neutrinos from the sun allow a direct evidence: window into the nuclear solar processes • Neutrinos no longer massless Light Element Fusion Reactions particles (though mass is very 2 + - 2 p + p → H + e + νe p + e + p → H + νe small) 99.75% 0.25% • Experimental evidence from 2H + p →3He + γ different phenomena: -5 Solar 85% ~15% ~10 % 3He + 3He →4He + 2p 3He + p →4He + e+ +ν Atmospheric e Accelerator 3He + 4He →7Be + γ Reactor 15.07% 0.02% • Data supports the interpretation 7 - 7 Be + e → Li + γ +νe that neutrinos oscillate. 7Li + p →α+ α 7Be + p →8B + γ 8 8 + B → Be* + e + νe R. Galea (Columbia University) SMU Physics Seminar March 26th, 2007 Solar neutrinos over full (pp) spectrum Gallium Chlorine SNO, SK • In particular, a precision, real-time measurement of the pp neutrino spectrum down to the keV range • Precision measurements of oscillation effect matter/vacuum dominated regimes • SSM uncertainty on the pp flux ~ 1% → aim for “1%” measurement • Insights into the inner working of the Sun. -
A Post-Buckminsterfullerene View of Carbon Chemistry
A POST-BUCKMINSTERFULLERENE VIEW OF CARBON CHEMISTRY Harold Kroto School of Chemistry and Molecular Sciences, University of Sussex, Brighton, BNI 9QJ UK Keywords: Cs0, Fullerenes, carbon particles INTRODUCTION The discovery of c60 Buckminsterfullerene, Fig 1, has its origins in a research programme involving synthetic chemistry, microwave spectroscopy and radioastronomyl. In 1915, at Sussex (with David Walton), the long chain polyyne H-CeC-CsC-CsN was synthesised and studied by microwave spectroscopy. Subsequently, with Takeshi Oka and NRC(0ttawa) astronomers, the molecule was discovered in space, Fig 2, by radioastronomy using the laboratory microwave frequencies. This discovery led on to the detection of the even longer carbon chain molecules HCTN, HCgN and HCl.lN in the space between the stars2. Further work aimed at understanding the formation of the chains in space focussed attention on the possibility that they are produced at the same time as carbon dust in red giant stars1,*. During experiments at Rice University in 1985 (with James Heath, Sean O'Brien, Robert Curl and Richard Smalley), designed to simulate the conditions in these stars and explore their capacity for carbon chain formation, the exciting discovery that C60 was remarkably stable was made3. It was found that under conditions where almost all the atoms in a carbon plasma had nucleated to form microparticles the molecule c60 remained behind - together with some CTO. This result was, as is now well 'known, rationalised on the basis of the closed cage structure shown in Fig 1. It was proposed that the geodesic and aromatic factors inherent in such a structure could account for the stability of the molecule. -
Metallofullerene and Fullerene Formation from Condensing Carbon Gas Under Conditions of Stellar Outflows and Implication to Star
Metallofullerene and fullerene formation from condensing carbon gas under conditions of stellar outflows and implication to stardust Paul W. Dunka,b,1, Jean-Joseph Adjizianc, Nathan K. Kaiserb, John P. Quinnb, Gregory T. Blakneyb, Christopher P. Ewelsc,1, Alan G. Marshalla,b,1, and Harold W. Krotoa,1 aDepartment of Chemistry and Biochemistry, Florida State University, Tallahassee, FL 32306; bIon Cyclotron Resonance Program, National High Magnetic Field Laboratory, Florida State University, Tallahassee, FL 32310; and cInstitut des Matériaux Jean Rouxel, Centre National de la Recherche Scientifique, Unité Mixte de Recherche 6502, Université de Nantes, BP 32229 Nantes, France Contributed by Harold W. Kroto, August 29, 2013 (sent for review June 13, 2013) Carbonaceous presolar grains of supernovae origin have long confirmed to exist in circumstellar and interstellar environments. been isolated and are determined to be the carrier of anomalous C60 and C70 were first unequivocally detected in a planetary 22Ne in ancient meteorites. That exotic 22Ne is, in fact, the decay nebula in 2010, which was thought to be hydrogen deficient (11). isotope of relatively short-lived 22Na formed by explosive nucleo- Thereafter, Buckminsterfullerene was detected in hydrogen- synthesis, and therefore, a selective and rapid Na physical trapping rich [including the least H-deficient R Coronae Borealis stars] mechanism must take place during carbon condensation in super- (12, 13) and oxygen-rich environments (14), as well as the ISM nova ejecta. Elucidation of the processes that trap Na and produce (15) and a protoplanetary nebula (16). Moreover, fullerenes large carbon molecules should yield insight into carbon stardust have been detected in a host of other circumstellar and in- enrichment and formation. -
AZMAN AIR CLASSES DANGEROUS GOODS 'Dangerous Goods' Are
AZMAN AIR CLASSES DANGEROUS GOODS ‘Dangerous goods’ are materials or items with hazardous properties Commonly Transported Explosives which, if not properly controlled, 1. Ammunition/cartridges present a potential hazard to human 2. Fireworks/pyrotechnics health and safety, infrastructure and/ 3. Flares or their means of transport. 4. Blasting caps / detonators 5. Fuse The transportation of dangerous 6. Primers goods is controlled and governed by a 7. Explosive charges (blasting, variety of different regulatory demolition etc) regimes, operating at both the 8. Detonating cord national and international levels. 9. Air bag inflators Prominent regulatory frameworks for 10. Igniters the transportation of dangerous 11. Rockets goods include the United Nations 12. TNT / TNT compositions Recommendations on the Transport 13. RDX / RDX compositions of Dangerous Goods, ICAO’s Technical 14. PETN / PETN compositions Instructions, IATA’s Dangerous Goods Regulations and the IMO’s International Maritime Dangerous Commonly Transported Gases Goods Code. Collectively, these 1. Aerosols regulatory regimes mandate how 2. Compressed air dangerous goods are to be handled, 3. Hydrocarbon gas-powered packaged, labelled and transported. devices 1. Explosives 4. Fire extinguishers 2. Gases 5. Gas cartridges 3. Flammable Liquids 6. Fertilizer ammoniating 4. Flammable Solids solution 5. Oxidizing Substances 7. Insecticide gases 6. Toxic & Infectious Substances 8. Refrigerant gases 7. Radioactive Material 9. Lighters 8. Corrosives 10. Acetylene / Oxyacetylene 9. Miscellaneous Dangerous 11. Carbon dioxide Goods 12. Helium / helium compounds 13. Hydrogen / hydrogen compounds 14. Oxygen / oxygen 21. Organochlorine pesticides compounds 22. Organophosphorus 15. Nitrogen / nitrogen pesticides compounds 23. Copper based pesticides 16. Natural gas 24. Esters 17. Oil gas 25. Ethers 18. -
Two Species of Electrons in Helium Discovered
Two species of electrons in helium discovered July 15, 2021 In news The scientists at Bangalore’s Indian Institute of Science (IISc) have discovered the existence of two species of few electron bubbles (FEBs) in superfluid helium for the first time. Key updates Scientists have experimentally observed FEBs for the first time and understood how they are created. The study was published in ‘Science Advances’. This is the first time scientists have shown the existence of two species of few electron bubbles (FEBs) in superfluid helium. The scientists applied a voltage pulse to a tungsten tip on the surface of liquid helium. They generated a pressure wave on the charged surface, using an ultrasonic transducer. This allowed them to create 8EBs (electron bubbles) and 6EBs, two species of FEBs containing 8 and 6 electrons. The study stated that, like how current flows without resistance in superconducting materials at very low temperatures, superfluid helium also conducts heat efficiently at very low temperatures. Defects in the system, called vortices, however, can lower its thermal conductivity. As FEBs are present at the core of such vortices, they can help in studying how vortices interact with each other. Single Electronic Bubble(SEB) As per the study, an electron injected into a superfluid form of helium creates a single electron bubble – a cavity free of helium atoms and containing only the electron. The shape of the bubble depends on the energy state of the electron. An electron bubble is the empty space created around a free electron in a cryogenic gas or liquid, such as neon or helium. -
Formation of Buckminsterfullerene (C60) in Interstellar Space
Formation of buckminsterfullerene ( ) C60 in interstellar space Olivier Berné1 and A. G. G. M. Tielens Leiden Observatory, Leiden University, P.O. Box 9513, NL- 2300 RA Leiden, The Netherlands Edited by Neta A. Bahcall, Princeton University, Princeton, NJ, and approved November 2, 2011 (received for review August 31, 2011) Buckminsterfullerene (C60) was recently confirmed as the largest region, at high angular resolution (Fig. 1). This measurement can molecule identified in space. However, it remains unclear how be used to derive the integrated intensity radiated by the nebula, and where this molecule is formed. It is generally believed that which can be used as a calibrator, to convert the Spitzer observa- C60 is formed from the buildup of small carbonaceous compounds tions of the PAHs and C60 bands into absolute chemical abun- in the hot and dense envelopes of evolved stars. Analyzing infrared dances of these species, allowing a quantitive study of PAH and observations, obtained by Spitzer and Herschel, we found that C60 C60 chemical evolution. is efficiently formed in the tenuous and cold environment of an interstellar cloud illuminated by strong ultraviolet (UV) radiation Measurement of the Far Infrared Integrated Intensity of Dust Emission I fields. This implies that another formation pathway, efficient at in the Nebula. The far infrared integrated intensity FIR was ex- low densities, must exist. Based on recent laboratory and theore- tracted by fitting the spectral energy distribution (SED) at each tical studies, we argue that polycyclic aromatic hydrocarbons are position in the cross-cut shown in Fig. 1. For these positions, we converted into graphene, and subsequently C60, under UV irradia- have used the brightnesses as measured by Herschel Photodetec- tion from massive stars. -
First-Principles Calculations of Helium Cluster Formation in Palladium Tritides
FIRST-PRINCIPLES CALCULATIONS OF HELIUM CLUSTER FORMATION IN PALLADIUM TRITIDES A Thesis Presented to The Academic Faculty by Pei Lin In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the School of Physics Georgia Institute of Technology August 2010 FIRST-PRINCIPLES CALCULATIONS OF HELIUM CLUSTER FORMATION IN PALLADIUM TRITIDES Approved by: Professor Mei-Yin Chou, Advisor Professor Andrew Zangwill School of Physics School of Physics Georgia Institute of Technology Georgia Institute of Technology Professor James Gole Professor David Sholl School of Physics School of Chemical and Biomolecular Georgia Institute of Technology Engineering Georgia Institute of Technology Professor Phillip N. First Date Approved: May 10, 2010 School of Physics Georgia Institute of Technology To my beloved family iii ACKNOWLEDGEMENTS I owe my sincere gratitude to all who have helped me, encouraged me, and believed in me through this challenging journey. Foremost, I am deeply indebted to my thesis advisor, Professor Mei-Yin Chou, for every advice and opportunity she provided me through the years of my education. Her exceptional insight and broad-minded guidance led me the way to be a critical-thinking and self-stimulating physicist, which would be my greatest asset in the future. I owe my sincere thanks to Professor Andrew Zangwill, Professor James Gole, Professor Phillip First, and Professor David Sholl for their precious time being in my thesis defense committee. I am thankful to our previous and current group members Dr. Amra Peles, Dr. Li Yang, Dr. Zhu Ma, Dr. Wolfgang Geist, Dr. Alexis Nduwinmana, Dr. Jia-An Yan, Dr. Wen-Ying Ruan, Dr. -
Reactions of Graphene Oxide and Buckminsterfullerene in the Aquatic Environment Yingcan Zhao Purdue University
Purdue University Purdue e-Pubs Open Access Dissertations Theses and Dissertations 8-2016 Reactions of graphene oxide and buckminsterfullerene in the aquatic environment Yingcan Zhao Purdue University Follow this and additional works at: https://docs.lib.purdue.edu/open_access_dissertations Part of the Environmental Engineering Commons Recommended Citation Zhao, Yingcan, "Reactions of graphene oxide and buckminsterfullerene in the aquatic environment" (2016). Open Access Dissertations. 896. https://docs.lib.purdue.edu/open_access_dissertations/896 This document has been made available through Purdue e-Pubs, a service of the Purdue University Libraries. Please contact [email protected] for additional information. Graduate School Form 30 Updated PURDUE UNIVERSITY GRADUATE SCHOOL Thesis/Dissertation Acceptance This is to certify that the thesis/dissertation prepared By Yingcan Zhao Entitled REACTIONS OF GRAPHENE OXIDE AND BUCKMINSTERFULLERENE IN THE AQUATIC ENVIRONMENT For the degree of Doctor of Philosophy Is approved by the final examining committee: Chad T. Jafvert Chair Timothy R. Filley Inez Hua Ronald F. Turco To the best of my knowledge and as understood by the student in the Thesis/Dissertation Agreement, Publication Delay, and Certification Disclaimer (Graduate School Form 32), this thesis/dissertation adheres to the provisions of Purdue University’s “Policy of Integrity in Research” and the use of copyright material. Approved by Major Professor(s): Chad T. Jafvert Approved by: Dulcy M. Abraham 6/21/2016 Head of the Departmental Graduate Program Date i REACTIONS OF GRAPHENE OXIDE AND BUCKMINSTERFULLERENE IN THE AQUATIC ENVIRONMENT A Dissertation Submitted to the Faculty of Purdue University by Yingcan Zhao In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy August 2016 Purdue University West Lafayette, Indiana ii To my parents and Liang, for their love, support and encouragement. -
Book of Abstracts
THE PHYSICS AND CHEMISTRY OF THE INTERSTELLAR MEDIUM Celebrating the first 40 years of Alexander Tielens' contribution to Science Book of Abstracts Palais des Papes - Avignon - France 2-6 September 2019 CONFERENCE PROGRAM Monday 2 September 2019 Time Speaker 10:00 Registration 13:00 Registration & Welcome Coffee 13:30 Welcome Speech C. Ceccarelli Opening Talks 13:40 PhD years H. Habing 13:55 Xander Tielens and his contributions to understanding the D. Hollenbach ISM The Dust Life Cycle 14:20 Review: The dust cycle in galaxies: from stardust to planets R. Waters and back 14:55 The properties of silicates in the interstellar medium S. Zeegers 15:10 3D map of the dust distribution towards the Orion-Eridanus S. Kh. Rezaei superbubble with Gaia DR2 15:25 Invited Talk: Understanding interstellar dust from polariza- F. Boulanger tion observations 15:50 Coffee break 16:20 Review: The life cycle of dust in galaxies M. Meixner 16:55 Dust grain size distribution across the disc of spiral galaxies M. Relano 17:10 Investigating interstellar dust in local group galaxies with G. Clayton new UV extinction curves 17:25 Invited Talk: The PROduction of Dust In GalaxIES C. Kemper (PRODIGIES) 17:50 Unravelling dust nucleation in astrophysical media using a L. Decin self-consistent, non steady-state, non-equilibrium polymer nucleation model for AGB stellar winds 19:00 Dining Cocktail Tuesday 3 September 2019 08:15 Registration PDRs 09:00 Review: The atomic to molecular hydrogen transition: a E. Roueff major step in the understanding of PDRs 09:35 Invited Talk: The Orion Bar: from ALMA images to new J. -
Ionization Dynamics of Helium Dimers in Fast Collisions with Heþþ
week ending PRL 106, 033201 (2011) PHYSICAL REVIEW LETTERS 21 JANUARY 2011 Ionization Dynamics of Helium Dimers in Fast Collisions with Heþþ J. Titze,1 M. S. Scho¨ffler,2 H.-K. Kim,1 F. Trinter,1 M. Waitz,1 J. Voigtsberger,1 N. Neumann,1 B. Ulrich,1 K. Kreidi,3 R. Wallauer,1 M. Odenweller,1 T. Havermeier,1 S. Scho¨ssler,1 M. Meckel,1 L. Foucar,4 T. Jahnke,1 A. Czasch,1 L. Ph. H. Schmidt,1 O. Jagutzki,1 R. E. Grisenti,1 H. Schmidt-Bo¨cking,1 H. J. Lu¨dde,5 and R. Do¨rner1,* 1Institut fu¨r Kernphysik, Goethe-Universita¨t Frankfurt am Main, Max-von-Laue-Str.1, 60438 Frankfurt, Germany 2Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California, 94720, USA 3GSI Helmholtzzentrum fu¨r Schwerionenforschung GmbH, Planckstr. 1, 64291 Darmstadt, Germany 4Max-Planck-Institut fu¨r Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany 5Institut fu¨r Theoretische Physik, Goethe-Universita¨t Frankfurt am Main, Max-von-Laue-Str. 1, 60438 Frankfurt, Germany (Received 23 September 2010; published 20 January 2011) By employing the cold target recoil ion momentum spectroscopy technique, we have investigated the þ þ (He , He ) breakup of a helium dimer (He2) caused by transfer ionization and double capture in collisions with alpha particles (E ¼ 150 keV=u). Surprisingly, the results show a two-step process as well as a one-step process followed by electron exchange. In addition, interatomic Coulombic decay [L. S. Cederbaum, J. Zobeley, and F. Tarantelli, Phys. Rev. Lett. 79, 4778 (1997).] is observed in an ion collision for the first time. -
Carbon-Based Nanomaterials/Allotropes: a Glimpse of Their Synthesis, Properties and Some Applications
materials Review Carbon-Based Nanomaterials/Allotropes: A Glimpse of Their Synthesis, Properties and Some Applications Salisu Nasir 1,2,* ID , Mohd Zobir Hussein 1,* ID , Zulkarnain Zainal 3 and Nor Azah Yusof 3 1 Materials Synthesis and Characterization Laboratory (MSCL), Institute of Advanced Technology (ITMA), Universiti Putra Malaysia, 43400 Serdang, Selangor, Malaysia 2 Department of Chemistry, Faculty of Science, Federal University Dutse, 7156 Dutse, Jigawa State, Nigeria 3 Department of Chemistry, Faculty of Science, Universiti Putra Malaysia, 43400 Serdang, Selangor, Malaysia; [email protected] (Z.Z.); [email protected] (N.A.Y.) * Correspondence: [email protected] (S.N.); [email protected] (M.Z.H.); Tel.: +60-1-2343-3858 (M.Z.H.) Received: 19 November 2017; Accepted: 3 January 2018; Published: 13 February 2018 Abstract: Carbon in its single entity and various forms has been used in technology and human life for many centuries. Since prehistoric times, carbon-based materials such as graphite, charcoal and carbon black have been used as writing and drawing materials. In the past two and a half decades or so, conjugated carbon nanomaterials, especially carbon nanotubes, fullerenes, activated carbon and graphite have been used as energy materials due to their exclusive properties. Due to their outstanding chemical, mechanical, electrical and thermal properties, carbon nanostructures have recently found application in many diverse areas; including drug delivery, electronics, composite materials, sensors, field emission devices, energy storage and conversion, etc. Following the global energy outlook, it is forecasted that the world energy demand will double by 2050. This calls for a new and efficient means to double the energy supply in order to meet the challenges that forge ahead.