26 results on '"Pearson, J."'
Search Results
2. Strong anisotropy in single atomic layer of Co and Fe and Pt(997)
- Author
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Ruihua Cheng, Pearson, J., Dongqi Li, and Fradin, F.Y.
- Subjects
Anisotropy -- Analysis ,Monomolecular films -- Magnetic properties ,Monomolecular films -- Structure ,Surface chemistry -- Research ,Physics - Abstract
The growth and magnetic properties of magnetic monolayers grown on a Pt(997) vicinal single crystal surface at room temperature is investigated. The magnetic easy axis of the atomic layers is perpendicular to the surface due to strong surface anisotropy.
- Published
- 2006
3. Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
- Author
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Fantina A. F., Chamel N., Pearson J. M., and Goriely S.
- Subjects
Physics ,QC1-999 - Abstract
The Brussels-Montreal equations of state of cold dense nuclear matter that have been recently developed are tested against various constraints coming from both nuclear physics and astrophysics. The nuclear physics constraints include the analysis of nuclear flow and kaon production in heavy-ion collision experiments, as well as recent microscopic many-body calculations of infinite homogeneous neutron matter. Astrophysical observations, especially recent neutron-star mass measurements, provide valuable constraints on the high-density part of the equation of state that is not accessible in laboratory experiments.
- Published
- 2014
- Full Text
- View/download PDF
4. Effect of mechanical processing on giant magnetoresistance in melt-spun Co-Cu ribbons
- Author
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Jiang, J.S., Pearson, J., Hinks, D., and Bader, S.D.
- Subjects
Cobalt alloys -- Analysis ,Copper alloys -- Analysis ,Magnetization -- Research ,Physics - Abstract
The impact of uniaxial deformation on the giant magnetoresistance (GMR) effect in cobalt-copper (Co-Cu) ribbons are examined in an experiment. Samples of free-standing ribbons created using the melt-spinning technique are used for the study. Test results show that the GMR effect is affected by the structural disorder and the resistivity of mechanical processing. In addition, it was observed that Co particles are not affected by postprecipitation deformation.
- Published
- 1997
5. Magnetic coupling of Fe/Mo/Fe and Co/Cu/Co sandwiches across wedged spacer layers
- Author
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Qiu, Z. Q., Pearson, J., and Bader, S.D.
- Subjects
Thin films, Multilayered -- Research ,Layer structure (Solids) -- Research ,Magnetism -- Research ,Physics - Abstract
The magnetic behavior of Fe/Mo/Fe and Co/Cu/Co sandwiches epitaxially grown on Mo(100) and Cu(100) single crystals were investigated using electron diffraction and in situ magneto-optic Kerr effect measurements. The results showed that there was an oscillatory behavior between ferromagnetic and antiferromagnetic coupling. This behavior originated from the interface between the magnetic and the spacer layers.
- Published
- 1993
6. Magnetic properties of ultrathin Fe films grown on stepped W(001) and Pd(001) substrates
- Author
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Choi, Hyuk J., Kawakami, R.K., Escorcia-Aparicio, J., Qiu, Z.Q., Pearson, J., Jiang, J.S., Li, Dongqi, Osgood, R.M., III, and Bader, S.D.
- Subjects
Magnetism -- Research ,Thin films -- Magnetic properties ,Iron -- Research ,Physics - Abstract
A study was conducted to analyze the magnetic characteristics of ultrathin iron films prepared on stepped W(001) and Pd(001) substrates. The substrates were mechanically polished with diamond-paste finish. Experimental results indicated that improvements in the Curie temperature correlated with the step-induced Pd moments that is supported by the increased surface magneto-optic Kerr effect signal on the stepped surface.
- Published
- 1999
7. Structural and magnetic studies of fcc Fe films with self-organized lateral modulation on striped Cu(110)-O(2x1) substrates
- Author
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Li, Dongqi, Diercks, Verena, Pearson, J., Jiang, J.S., and Bader, S.D.
- Subjects
Thin films -- Research ,Iron -- Research ,Copper -- Research ,Ferromagnetism -- Research ,Physics - Abstract
Face-centered cubic Fe was grown onto a novel Cu(110) substrate with ordered Cu-O stripes. Results showed that the growth mode was layer-by-layer and was better than either clean or oxygen-saturated Cu(110). It was postulated that the Fe films grow conformationally onto the original striped substrate. Lateral long-range ordering of the stripe-like structure on Fe was retained up tp 6-7 ML. These films were ferromagnetic with in-plane magnetic anisotropy.
- Published
- 1999
8. Field and stress dependence of the irreversible magnetization changes in pure iron
- Author
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Pearson, J. and Squire, P.T.
- Subjects
Ferromagnetic materials -- Observations ,Stress relieving (Materials) -- Observations ,Iron -- Fatigue ,Physics - Abstract
Several studies have examined the effects of stress on the magnetic properties of ferromagnetic materials. Pravdin considered the effects of low-magnitude cyclic stress, separating irreversible and reversible changes following several cycles. The work is extended to higher magnitude stresses, and it is shown how the peak position of DeltaMIRR alters with the magnitude and sign of the applied stress, in a sample of 99.99% pure iron.
- Published
- 1998
9. Spin polarization of the conduction bands and secondary electrons of Gd(0001)
- Author
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Dongqi, Li, Pearson, J., Bader, S.D., McIlroy, D.N., Waldfried, C., and Dowben, P.A.
- Subjects
Photoemission -- Research ,Electrons -- Analysis ,Physics - Published
- 1996
10. Magnetic and structural instabilities of ferromagnetic and antiferromagnetic Fe/Cu(100)
- Author
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Li, Dongqi, Freitag, M., Pearson, J., Qiu, Z.Q., and Bader, S.D.
- Subjects
Thin films -- Magnetic properties ,Iron -- Magnetic properties ,Copper -- Magnetic properties ,Physics - Abstract
Examination of the ferromagnetic and antiferromagnetic phases of the Fe wedges epitaxially grown on Cu(100) helps investigate the interaction between magnetic and structural instabilities. Fcc Fe films with 6-11 monolayer (ML) exhibit antiferromagnetic phase and a ferromagnetic surface. Antiferromagnetic phase is absent in films grown below 200 K, but they are ferromagnetic and undergo a spin-reorientation transition at about 6 ML. A new magnetic phase diagram based on thickness and growth temperature is developed for the growth of Fe/Cu(100).
- Published
- 1994
11. Ferromagnetic microdisks as carriers for biomedical applications
- Author
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Rozhkova, E.A., Novosad, V., Kim, D.-H., Pearson, J., Divan, R., Rajh, T., and Bader, S.D.
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Biophysics -- Research ,Ferromagnetism -- Analysis ,Magnetization -- Analysis ,Tumors -- Care and treatment ,Physics - Abstract
The fabrication process, magnetic behavior, as well as the surface modification of ferromagnetic microdisks suspended in aqueous solution is described. The method has helped in fabricating suitable magnetic carriers with excellent size tolerance and the particles have a magnetic core covered with gold on each side to provide stability at ambient conditions as well as biocompatibility and selective adhesion functions.
- Published
- 2009
12. The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI)
- Author
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de Graauw, Th., Whyborn, N., Caux, E., Phillips, T., Stutzki, J., Tielens, A., Güsten, R., Helmich, F., Luinge, W., Martin-Pintado, J., Pearson, J., Planesas, P., Roelfsema, P., Saraceno, P., Schieder, R., Wildeman, K., Wafelbakker, K., Pagani, L., Gerin, M., and Astronomy
- Subjects
Heterodyne ,Physics ,Spectrometer ,Frequency band ,business.industry ,Local oscillator ,Astrophysics::Instrumentation and Methods for Astrophysics ,General Engineering ,Astronomy and Astrophysics ,Radio spectrum ,Optics ,Space and Planetary Science ,Heterodyne detection ,Multi-band device ,business ,Astrophysics::Galaxy Astrophysics ,Noise (radio) - Abstract
The Heterodyne Instrument for the Far-Infrared (HIFI) is a single sky-pixel, high-resolution (>300.000), spectrometer for ESA's Herschel Space Observatory. The instrument is designed to provide a wide and continuous frequency coverage with a velocity resolved resolution and a high sensitivity. This allows detailed investigations of a wide variety of astronomical sources, ranging from solar system objects, star formation regions to nuclei of galaxies. The frequency bands cover many emission and absorption lines of molecules, like H/sub 2/O, and atomic and ionic lines, like CII, NII. The instrument comprises of 5 frequency bands covering 480-150 GHz with SIS mixers and a sixth dual band for the 1410-1910 GHz range with Hot Electron Bolometer Mixers. The Local Oscillator (LO) subsystem consists of a Ka-band synthesiser followed by 14 chains of frequency multipliers, 2 for each frequency band. Each frequency band has two mixers operating on orthogonal polarisations. All mixers are designed to have a noise performance close to the quantum noise limit. One frequency band is operated at a time. Modular design of the Focal Plane Unit, with a common optical path for all the mixer bands, and of the Local Oscillator Unit with a common LO Source Unit for all the LO chains, make the instrument very compact. A pair of Auto-Correlators and a pair of Acousto-Optic spectrometers process the two IF signals from the dual-polarisation front-ends and provide instantaneous frequency coverage of 4 GHz, resulting in a set of resolutions (140 KHz to 1 MHz), better than
- Published
- 2008
13. General equivalent circuit for intermediate band devices: potentials currents and electroluminescence
- Author
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Luque, A., Marti, A., Stanley, C., Lopez, N., Cuadra, L., McKee, A., Pearson, J. L., and Zhou, D.
- Subjects
Electroluminescence -- Analysis ,Fermium -- Analysis ,Physics - Abstract
Circuit representation of the equations in which the voltage differences correspond to the quasi-fermi level split between bands was presented. Analysis of the circuit reveals that the quasi-fermi levels of he conduction and intermediate bands are separated.
- Published
- 2004
14. Placement of epitaxial magnetic Co dots on Ru(0001) via substrate modifications
- Author
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Dongqi Li, Ruihua Cheng, Chengtao Yu, Pearson, J., Fradin, F.Y., and Bader, S.D.
- Subjects
Cobalt -- Magnetic properties ,Ruthenium -- Magnetic properties ,Physics - Abstract
The control of the placement of the Co dots by the surface morphological features on Ru(0001) substrates is discussed. The dots are aligned along the edges of the surface features (~4-100 nm deep) and form dot chains, wires, arrays and dots around lithographic patterns on modification of the Ru surface morphology via scratches or e-beam lithography.
- Published
- 2004
15. Magnetic domains and magnetostatic interactions of self-assembled Co dots
- Author
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Yu, Chengtao, Pearson, J., and Li, Dongqi
- Subjects
Magnetostatics -- Research ,Physics - Abstract
The magnetic properties of the self-assembled Co dots and dot pairs/chains are studied with magnetic force microscopy (MFM) and micromagnetic calculations. The inter-dot magnetostatic coupling, modeled with a dot pair, introduces a uniaxial anisotropy with easy axis along the pair/chain direction.
- Published
- 2002
16. A high-resolution line survey of IRC+10216 with Herschel/HIFI. First results: Detection of warm silicon dicarbide (SiC2)
- Author
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Cernicharo, J., Waters, L.B.F.M., Decin, L., Encrenaz, P., Tielens, A. G. G. M., Agúndez, M., De Beck, E., Müller, H. S. P., Goicoechea, J. R., Barlow, M.J., Benz, A., Crimier, N., Daniel, F., Di Giorgio, A. M., Fich, M., Gaier, T., García-Lario, P., de Koter, A., Khouri, T., Liseau, R., Lombaert, R., Erickson, N., Pardo, J. R., Pearson, J. C., Shipman, R., Sánchez Contreras, C., Teyssier, D., Astrophysics, Afd Astrophysics begr 1/1/17, Centro de Astrobiología, Consejo Superior de Investigaciones Científicas (CSIC)/Instituto Nacional de Técnica Aeroespacial (INTA) (CAB), Astronomical Institute Anton Pannekoek, University of Amsterdam, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Instrumentation et télédétection, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres (LERMA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY), Leiden Observatory, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Physikalisches Institut, Universität zu Köln, University College of London [London] (UCL), Institute for Astronomy, Department of Physics, ETH Zürich, Istituto di Fisica dello Spazio Interplanetario (IFSI), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Department of Physics and Astronomy, University of Waterloo, Jet Propulsion Laboratory, California Institute of Technology (JPL), European Space Astronomy Centre (ESAC), Agence Spatiale Européenne = European Space Agency (ESA), Department of Radio and Space Science, Chalmers University of Technology, Department of Astronomy, University of Massachusetts, SRON Netherlands Institute for Space Research, Low Energy Astrophysics (API, FNWI), Astrophysics, and Afd Astrophysics begr 1/1/17
- Subjects
Silicon ,chemistry.chemical_element ,FOS: Physical sciences ,Astrophysics ,stars: AGB and post-AGB ,SUBMILLIMETER HCN LASER ,COLOGNE DATABASE ,Quality (physics) ,CHEMISTRY ,LABORATORY MEASUREMENT ,Line (formation) ,stars: individual: IRC+10216 ,Physics ,ENVELOPE ,Range (particle radiation) ,Spectrometer ,astrochemistry ,Hydrogen molecule ,Resolution (electron density) ,Astronomy and Astrophysics ,Rotational temperature ,Astrophysics - Astrophysics of Galaxies ,BURE OBSERVATIONS ,CO ,stars: carbon ,chemistry ,Space and Planetary Science ,MOLECULAR-SPECTROSCOPY ,Astrophysics of Galaxies (astro-ph.GA) ,stellar evolaution [astronomy and astrophysics] ,DUST FORMATION ZONE ,EMISSION ,AGB stars ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,line: identification - Abstract
We present the first results of a high-spectral-resolution survey of the carbon-rich evolved star IRC+10216 that was carried out with the HIFI spectrometer onboard Herschel. This survey covers all HIFI bands, with a spectral range from 488 to 1901GHz. In this letter we focus on the band-1b spectrum, in a spectral range 554.5-636.5GHz, where we identified 130 spectral features with intensities above 0.03 K and a signal-to-noise ratio >5. Detected lines arise from HCN, SiO, SiS, CS, CO, metal-bearing species and, surprisingly, silicon dicarbide (SiC2). We identified 55 SiC2 transitions involving energy levels between 300 and 900 K. By analysing these rotational lines, we conclude that SiC2 is produced in the inner dust formation zone, with an abundance of ~2x10^-7 relative to molecular hydrogen. These SiC2 lines have been observed for the first time in space and have been used to derive an SiC2 rotational temperature of ~204 K and a source-averaged column density of ~6.4x10^15 cm^-2. Furthermore, the high quality of the HIFI data set was used to improve the spectroscopic rotational constants of SiC2., A&A HIFI Special Issue, 2010
- Published
- 2010
17. Hydrides in Young Stellar Objects: Radiation tracers in a protostar-disk-outflow system
- Author
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Benz, A. O., Bruderer, S., van Dishoeck, E. F., Staeuber, P., Wampfler, S. F., Melchior, M., Dedes, C., Wyrowski, F., Doty, S. D., van der Tak, F., Baechtold, W., Csillaghy, A., Megej, A., Monstein, C., Soldati, M., Bachiller, R., Baudry, A., Benedettini, M., Bergin, E., Bjerkeli, P., Blake, G.A., Bontemps, S., Braine, J., Caselli, P., Cernicharo, J., Codella, C., Daniel, F., di Giorgio, A. M., Dieleman, P., Dominik, C., Encrenaz, P., Fich, M., Fuente, A., Giannini, T., Goicoechea, J. R., de Graauw, Th., Helmich, F., Herczeg, G. J., Herpin, F., Hogerheijde, M. R., Jacq, T., Jellema, W., Johnstone, D., Jorgensen, J. K., Kristensen, L. E., Larsson, B., Lis, D., Liseau, R., Marseille, M., McCoey, C., Melnick, G., Neufeld, D., Nisini, B., Olberg, M., Ossenkopf, V., Parise, B., Pearson, J. C., Plume, R., Risacher, C., Santiago-Garcia, J., Saraceno, P., Schieder, R., Shipman, R., Stutzki, J., Tafalla, M., Tielens, A. G. G. M., van Kempen, T. A., Visser, R., Yildiz, U. A., Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1, Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB), Civilisations atlantiques & Archéosciences (C2A), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Ministère de la Culture et de la Communication (MCC)-Université de Rennes 2 (UR2), Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS)-Université de Nantes - UFR Histoire, Histoire de l'Art et Archéologie (UFR HHAA), Université de Nantes (UN)-Université de Nantes (UN), SRON Netherlands Institute for Space Research (SRON), Université de Nantes - UFR Histoire, Histoire de l'Art et Archéologie (UFR HHAA), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Ministère de la Culture et de la Communication (MCC), Low Energy Astrophysics (API, FNWI), and Astronomy
- Subjects
H3O+ ,Astronomy ,Young stellar object ,FOS: Physical sciences ,Context (language use) ,Astrophysics ,Radiation ,01 natural sciences ,7. Clean energy ,W3IRS5 ,photon-dominated region ,CHEMISTRY ,0103 physical sciences ,Protostar ,H2O+ ,010306 general physics ,010303 astronomy & astrophysics ,QB ,Line (formation) ,Physics ,stars: formation ,SPECTROSCOPY ,astrochemistry ,DR21 ,Star formation ,[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Astronomy and Astrophysics ,REGIONS ,[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Astrophysics - Astrophysics of Galaxies ,stars: massive ,13. Climate action ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,ComputingMethodologies_DOCUMENTANDTEXTPROCESSING ,submillimeter: ISM ,Outflow ,Absorption (chemistry) ,line: identification - Abstract
Context: Hydrides of the most abundant heavier elements are fundamental molecules in cosmic chemistry. Some of them trace gas irradiated by UV or X-rays. Aims: We explore the abundances of major hydrides in W3 IRS5, a prototypical region of high-mass star formation. Methods: W3 IRS5 was observed by HIFI on the Herschel Space Observatory with deep integration (about 2500 s) in 8 spectral regions. Results: The target lines including CH, NH, H3O+, and the new molecules SH+, H2O+, and OH+ are detected. The H2O+ and OH+ J=1-0 lines are found mostly in absorption, but also appear to exhibit weak emission (P-Cyg-like). Emission requires high density, thus originates most likely near the protostar. This is corroborated by the absence of line shifts relative to the young stellar object (YSO). In addition, H2O+ and OH+ also contain strong absorption components at a velocity shifted relative to W3 IRS5, which are attributed to foreground clouds. Conclusions: The molecular column densities derived from observations correlate well with the predictions of a model that assumes the main emission region is in outflow walls, heated and irradiated by protostellar UV radiation., Comment: Astronomy and Astrophysics Letters, in press
- Published
- 2010
18. Status of the TRIUMF annular chamber for the tracking and identification of charged particles (TACTIC).
- Author
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Fülöp, Zsolt, Gyürky, György, Somorjai, Endre, Ruprecht, G., Gigliotti, D., Amaudruz, P., Buchmann, L., Fox, S. P., Fulton, B. R., Kirchner, T., Laird, A. M., Mumby-Croft, P. D., Openshaw, R., Pavan, M. M., Pearson, J., Sheffer, G., and Walden, P.
- Abstract
TACTIC (TACTIC web site: http://tactic.triumf.ca) is a new detector for low-energy nuclear reactions currently under development at TRIUMF. The cylindrical ionization chamber allows three-dimensional reconstruction of particle tracks by means of a two-dimensional anode array combined with a TOF measurement of the drift electrons. In addition, the integrated charge for each pulse provides information about the energy loss of the particle and therefore allows a better identification of the nuclear species producing the track. The geometry of TACTIC covers a large angular range permitting the measurement of differential cross-sections over a large solid angle. It will be ideal for investigations of nuclear processes pertinent to the field of nuclear astrophysics. [ABSTRACT FROM AUTHOR]
- Published
- 2006
- Full Text
- View/download PDF
19. Recent progress in mass predictions.
- Author
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Gross, Carl J., Nazarewicz, Witold, Rykaczewski, Krzysztof P., Goriely, S., Samyn, M., Pearson, J. M., and Khan, E.
- Abstract
We review the latest efforts devoted to the global prediction of atomic masses. Special attention is paid to the new developments made within the Hartree-Fock-Bogolyubov framework. So far, 9 HFB mass tables based on different parametrizations of the effective interactions in the Hartree-Fock and pairing channels have been published. We analyze their ability to reproduce experimental masses as well as nuclear-matter and giant-resonance properties. The possibility to derive within the HFB framework a universal effective interaction that can describe all known properties of the nuclei (including their masses) and of asymmetric nuclear matter is critically discussed. [ABSTRACT FROM AUTHOR]
- Published
- 2005
- Full Text
- View/download PDF
20. Heavy ion radiative capture: 12C(12C,γ).
- Author
-
Jenkins, D. G., Fulton, B. R., Pearson, J., Lister, C. J., Carpenter, M. P., Freeman, S., Hammond, N., Janssens, R. V. F., Khoo, T. L., Lauritsen, T., Moore, E. F., Wuosmaa, A. H., Fallon, P., Görgen, A., Macchiavelli, A. O., McMahan, M., Freer, M., and Haas, F.
- Subjects
RESEARCH ,LABORATORIES ,HEAVY ions ,RADIATIVE capture ,PHYSICS - Abstract
The heavy ion radiative capture reaction 12C(12C,γ) has been investigated around a beam energy of 16 MeV. The total cross-section has been measured with the Fragment Mass Analyser at Argonne National Laboratory and found to be somewhat larger than has previously been measured. A subsequent measurement with the Gammasphere array has shown that a considerable proportion of this extra cross-section relates to a highly non-statistical decay through high-lying states in 24Mg. © 2004 American Institute of Physics [ABSTRACT FROM AUTHOR]
- Published
- 2004
- Full Text
- View/download PDF
21. Electron-beam tip/sample heating device for a scanning tunneling microscopy.
- Author
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Ding, H. F., Pearson, J. E., Dongqi Li, Ruihua Cheng, Fradin, F. Y., and Bader, S. D.
- Subjects
- *
ELECTRON beams , *ELECTRON optics , *ELECTRONICS , *PARTICLE beams , *SCANNING tunneling microscopy , *SCANNING probe microscopy , *SCIENTIFIC apparatus & instruments , *PHYSICS - Abstract
We present an electron-beam heating device for a scanning tunneling microscopy (STM) that can be used for heating both the STM tip and the sample to 2200 K. Mounted on a linear bellows with electrical feedthroughs, the device can be readily installed into the transfer path of a vacuum load lock. We demonstrate the heating capability of the device by flash cleaning Ru(0001) and Fe(001) crystals, and W tips. The flash-cleaned W tips are coated with Fe and further used for spin-polarized imaging of the Mn/Fe(001) system. [ABSTRACT FROM AUTHOR]
- Published
- 2005
- Full Text
- View/download PDF
22. Recent progress in mass predictions.
- Author
-
Goriely, S., Samyn, M., Pearson, J. M., and Khan, E.
- Subjects
MASS (Physics) ,NUCLEAR reactions ,HARTREE-Fock approximation ,NUCLEAR physics ,PHYSICS - Abstract
We review the latest efforts devoted to the global prediction of atomic masses. Special attention is paid to the new developments made within the Hartree-Fock-Bogolyubov framework. So far, 9 HFB mass tables based on different parametrizations of the effective interactions in the Hartree-Fock and pairing channels have been published. We analyze their ability to reproduce experimental masses as well as nuclear-matter and giant-resonance properties. The possibility to derive within the HFB framework a universal effective interaction that can describe all known properties of the nuclei (including their masses) and of asymmetric nuclear matter is critically discussed. [ABSTRACT FROM AUTHOR]
- Published
- 2005
- Full Text
- View/download PDF
23. Origin of recoil hysteresis loops in Sm–Co/Fe exchange-spring magnets.
- Author
-
Choi, Y., Jiang, J. S., Pearson, J. E., Bader, S. D., and Liu, J. P.
- Subjects
PROPERTIES of matter ,MAGNETICS ,PHYSICS ,PHYSICAL sciences ,ANISOTROPY - Abstract
Open recoil loops are often interpreted as a consequence of a breakdown in exchange coupling and attributed to the decoupled soft phase in exchange-coupled permanent magnets. However, in element-specific recoil loop measurements on Sm–Co/Fe exchange spring magnets, the authors found that the open recoil loops were present not only in the soft (Fe) layer but also in the hard (Sm–Co) layer, and were not a consequence of exchange coupling breakdown between the soft and hard layers. Comparison between the experimental results and micromagnetic calculations reveals that the observed open recoil loops originate from the anisotropy variations in the Sm–Co layer. [ABSTRACT FROM AUTHOR]
- Published
- 2007
- Full Text
- View/download PDF
24. Enhanced spin injection polarization in Co/Cu/Co nonlocal lateral spin valves.
- Author
-
Ji, Y., Hoffmann, A., Pearson, J. E., and Bader, S. D.
- Subjects
SPIN valves ,ELECTRODES ,INTERFACES (Physical sciences) ,SURFACES (Physics) ,DIFFUSION ,PHYSICS - Abstract
Nonlocal spin injection is demonstrated in Co/Cu/Co lateral spin valves. Measurement of a series of structures with varying Cu length between the Co electrodes permits a direct determination of both the Cu spin diffusion length λ
s and the spin injection polarization P at the Co/Cu interface. The value of λs is 200±20 nm at 10 K and >=110 nm at 300 K, which is shorter than previously reported, due to the possible presence of impurities in the Cu. However, the value of P is >7%, which is improved compared with previous reports of 2%, which is attributed to a higher interfacial quality. [ABSTRACT FROM AUTHOR]- Published
- 2006
- Full Text
- View/download PDF
25. The r-process nucleosynthesis during the decompression of neutronised matter
- Author
-
Pearson, J [Dept. de Physique, Universite de Montreal, Montreal (Quebec), H3C 3J7 (Canada)]
- Published
- 2011
- Full Text
- View/download PDF
26. Improvements of the DRAGON recoil separator at ISAC
- Author
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Vockenhuber, C., Buchmann, L., Caggiano, J., Chen, A.A., D’Auria, J.M., Davis, C.A., Greife, U., Hussein, A., Hutcheon, D.A., Ottewell, D., Ouellet, C.O., Parikh, A., Pearson, J., Ruiz, C., Ruprecht, G., Trinczek, M., and Zylberberg, J.
- Subjects
- *
PHYSICS , *NUCLEAR energy , *NUCLEAR warfare , *ANALOG resonance - Abstract
Abstract: The DRAGON (Detector of Recoils And Gammas Of Nuclear reactions) is used to measure radiative proton and alpha capture reaction rates involving both stable and radioactive, heavy-ion reactants at the TRIUMF-ISAC high intensity radioactive beam facility. Completed in 2001 it has been used for several challenging studies for nuclear astrophysics, e.g. 12C(α, γ)16O, 21Na(p, γ)22Mg, 26gAl(p, γ)27Si and 40Ca(α, γ)44Ti. Since initial operation, a number of improvements have been incorporated which are described here. These include a beam centering monitor based on a CCD camera, a mechanical iris to skim of beam halo, a solid state stripper acting as a charge state booster for beams with A ≳30, beta and gamma detectors to monitor beam intensity and to determine beam contamination in experiments with radioactive beam and the ionization chamber for both recoil identification and isobar separation. [Copyright &y& Elsevier]
- Published
- 2008
- Full Text
- View/download PDF
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