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Oxide ceramics under extreme pressure and radiation conditions
Oxide ceramics under extreme pressure and radiation conditions

The Potassium Promoter Function in the
The Potassium Promoter Function in the

... The interaction of potassium and oxygen, individually and as coadsorbates with graphite, was studied experimentallyand theoretically. In the experiments the sticking of oxygen was investigatedat different K coverages. The extremely low sticking coefficient for chemisorptionldissociation of dioxygen ...
Optical pumping studies of vibrational energy transfer
Optical pumping studies of vibrational energy transfer

... understood.5–11 V – V exchange rates between high vibrational levels of CO and air species have not been experimentally measured. In this paper we present measurements of the vibrational state distribution functions 共VDFs兲 of N2, O2, and CO in gas mixtures optically pumped by a CO laser at pressures ...
containing complexes of aromatic amino acids
containing complexes of aromatic amino acids

... Cu(II)-containing bis-complex of (a) tryptophan, (b) tyrosine, and (c) phenylalanine (unspecified Cu isotope will hereafter be understood to be 63Cu; the dissociation chemistries of the 65Cu-containing complexes were used for verification). The CID of [CuII(Trp)2] 2+ (Fig. 1a) reveals only products o ...
Impact of Ionizing Radiation on 4H-SiC Devices
Impact of Ionizing Radiation on 4H-SiC Devices

Gas-Phase Reactions of Fe (CH2O)+ and Fe (CH2S)+ with Small
Gas-Phase Reactions of Fe (CH2O)+ and Fe (CH2S)+ with Small

... dissociation, specific ion-molecule reactions, and use of labeled compounds, and experimental bond energies were obtained by using ion-molecule bracketing and competitive collisioninduced dissociation methods. Formaldehyde was chosen since it is the simplest hydrocarbon containing oxygen, and an und ...
Absorption of high-energy gamma rays in Cygnus X-3
Absorption of high-energy gamma rays in Cygnus X-3

The X-ray emission from shock cooling zones in O star winds
The X-ray emission from shock cooling zones in O star winds

Coronene and pyrene (5, 7)-member ring defects: Infrared spectra
Coronene and pyrene (5, 7)-member ring defects: Infrared spectra

... ionization is very small at those wavelengths. Also in this region the changes by the defects in intensities and positions of the lines can be found. Thus we notice in all areas of the spectra more significant deviations as in previous works. Yu & Nyman (2012) has raised the suspicion that there is ...
Predissociation dynamics of lithium iodide
Predissociation dynamics of lithium iodide

... Alkali halide diatomics were among the first molecules to be studied by femtosecond spectroscopy in the gas phase. Their lowest electronic excitations mostly lie in the visible or ultraviolet spectral range and are therefore well accessible by femtosecond lasers. Alkali halides are special in that t ...
university of oslo
university of oslo

... gallate, mixed conductors, and alkaline earth cerates which dissolve protons and become proton conductors at high temperatures. A revision of the book from 1972 as such is thus utopic in many respects. In the early 1990s Kofstad decided to author a new text that represented a development of the gene ...
Ab initio MCDHF calculations of electron
Ab initio MCDHF calculations of electron

... polynomial factors r −3 in the Hamiltonian (see section VI), which in turn strongly favor electronic orbitals with low angular momenta (predominantly s and p symmetries), since their densities are higher in the proximity of the nucleus. The typical distances for the hyperfine interaction are the rad ...
Vicky Kaspi Chandra Anomalous X-ray Pulsars Fotis Gavriil
Vicky Kaspi Chandra Anomalous X-ray Pulsars Fotis Gavriil

... – How are SGRs and AXPs related? One evolves to the other? – How are both related to high-B radio pulsars and other neutron stars? – Distinguishing property: Age? Mass? ...
Association of Nitrate Ion with Metal Cations in Aqueous Solution: a
Association of Nitrate Ion with Metal Cations in Aqueous Solution: a

... Abstract. Ion association in aqueous solutions of varied concentrations of LiNO3 , NaNO3 , Ca(NO3 ) 2 , Sr(NO3 ) 2 , Ba(NO3 ) 2 , Mn(NO3 )2 , Co(NO3 ) 2 , Ni(NO3 ) 2 , Cu(NO3 ) 2 , Zn(NO3 ) 2 , and Cd(NO3 ) 2 was studied by means of UV spectrometry. In all cases, except for Zn(NO 3 ) 2 (aq), the pri ...
Numerical solution of the radiative transfer equation: X
Numerical solution of the radiative transfer equation: X

幻灯片 1
幻灯片 1

... Nuclei contain positive protons and uncharged neutrons. The number of protons is the atomic number (Z) of an element. Electrostatic attractive force: Electrons are attracted to Nucleus The attractive strong interaction between protons and neutrons is opposed by electrostatic repulsion between proton ...
The Milky Way-Pulsars and Isolated Neutron Stars
The Milky Way-Pulsars and Isolated Neutron Stars

... on old V-2 (captured in Germany after the World War II) and Aerobee rockets, they were the first who detected X-rays from the very hot gas in the solar corona. However, the intensity of this radiation was found to be a factor 106 lower than that measured at optical wavelengths. In the late 1 X-rays ...
Journal - AIMS Lab
Journal - AIMS Lab

... Morse, Coulombic and three-body bending terms to construct the potential energy landscape. The calculation of electrostatic interactions between pair of ions is carried out using the three-dimensional Ewald summation method. In addition, the core-shell model is applied to effectively reproduce the po ...
Translation of rod-like template sequences into homochiral
Translation of rod-like template sequences into homochiral

The LDA+U Approach: A Simple Hubbard Correction - cond
The LDA+U Approach: A Simple Hubbard Correction - cond

chemistry - My Study materials – Kumar
chemistry - My Study materials – Kumar

... reactive. For example, hydrogen, oxygen, chlorine, etc. However, atoms of some elements, which are non-reactive, exist in free-state in nature. For example helium, neon, argon, etc. Usually atoms are exist in following two forms • In the form of molecules • In the form of ions Prepared by: M. S. Kum ...
Complex defects
Complex defects

... which dissolve protons and become proton conductors at high temperatures. A revision of the book from 1972 as such is thus unrealistic in many respects. In the early 1990s Kofstad decided to author a new text that represented a development of the general and theoretical first part of the former book ...
How to Make the σ0π2 Singlet the Ground State of Carbenes
How to Make the σ0π2 Singlet the Ground State of Carbenes

RIKEN Accelerator Progress Report
RIKEN Accelerator Progress Report

... as the detection system. Contamination of light elements in GaAs, Sb-doped Si and other semiconductor materials of industrial importance were successfully determined. Bromoperiodol labeled with 77 Br was prepared for the study on the dopamine receptor in the brain. In the field of radiation chemistr ...
Chapter 10 Chemical Bonding Theories
Chapter 10 Chemical Bonding Theories

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Metastable inner-shell molecular state



Metastable Innershell Molecular State (MIMS) is a class of ultra-high-energy short-lived molecules have the binding energy up to 1,000 times larger and bond length up to 100 times smaller than typical molecules. MIMS is formed by inner-shell electrons that are normally resistant to molecular formation. However, in stellar conditions, the inner-shell electrons become reactive to form molecular structures (MIMS) from combinations of all elements in the periodic table. MIMS upon dissociation can emit x-ray photons with energies up to 100 keV at extremely high conversion efficiencies from compression energy to photon energy. MIMS is predicted to exist and dominate radiation processes in extreme astrophysical environments, such as large planet cores, star interiors, and black hole and neutron star surroundings. There, MIMS is predicted to enable highly energy-efficient transformation of the stellar compression energy into the radiation energy.The right schematic illustration shows the proposed four stages of the K-shell MIMS (K-MIMS) formation and x-ray generation process. Stage I: Individual atoms are subjected to the stellar compression and ready for absorbing the compression energy. Stage II: The outer electron shells fuse together under increasing ""stellar"" pressure. Stage III: At the peak pressure, via pressure ionization K-shell orbits form the K-MIMS, which is vibrationally hot and encapsulated by a Rydberg-like pseudo-L-Shell structure. Stage IV: The K-MIMS cools down by ionizing (""boiling-off"") a number of pseudo-L-shell electrons and subsequent optical decay by emitting an x-ray photon. The dissociated atoms return their original atoms states and are ready for absorbing the compression energy.MIMS also can be readily produced in laboratory and industrial environments, such as hypervelocity particle impact, laser fusion and z-machine. MIMS can be exploited for highly energy-efficient production of high intensity x-ray beams for a wide range of innovative applications, such as photolithography, x-ray lasers, and inertial fusion.
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