Localization of 4 f State in YbRh2Si2 under Magnetic Field and High Pressure: Comparison with CeRh2Si2

2006 ◽  
Vol 75 (11) ◽  
pp. 114709 ◽  
Author(s):  
G. Knebel ◽  
R. Boursier ◽  
E. Hassinger ◽  
G. Lapertot ◽  
P. G. Niklowitz ◽  
...  
Keyword(s):  
Magnetic Field ◽  
High Pressure

scholarly journals A Novel Approach to Protein Crystallization: Use of a Magnetic Field and High-Pressure

2004 ◽  
Vol 44 (2) ◽  
pp. 58-63
Author(s):  
Gen SAZAKI ◽  
Shin-ichiro YANAGIYA ◽  
Yoshihisa SUZUKI ◽  
Satoru MIYASHITA ◽  
Takao SATO ◽  
...  
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Protein Crystallization ◽  
Novel Approach

The microinstabilities of a high-β plasma flow with a non-uniform velocity profile

1980 ◽  
Vol 24 (3) ◽  
pp. 385-407 ◽  
Author(s):  
A. B. Mikhailovskii ◽  
V. A. Klimenko
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Velocity Profile ◽  
Kinetic Analysis ◽  
Plasma Flow ◽  
Large Family ◽  
Larmor Radius ◽  
Helmholtz Instability ◽  
Uniform Velocity ◽  
Pressure Plasma

The microinstabilities of a high-pressure plasma moving along a magnetic field with a non-uniform velocity profile are investigated. A similar problem was studied earlier by Dobrowolny on the basis of hydromagnetic equations with an oblique viscosity tensor. The present paper, unlike Dobrowolny's work, gives a kinetic analysis. Perturbations with transverse wavelength both larger and smaller than the ion Larmor radius are considered. The analysis indicates that there is a large family of microinstabilities of the ‘drift’ type whose mechanism differs from the classical Kelvin–Helmholtz instability.

Design of High Pressure Apparatus to Use at Low Temperature and High magnetic Field

1993 ◽  
Vol 32 (S1) ◽  
pp. 349 ◽  
Author(s):  
Gendo Oomi ◽  
Tomoko Kagayama ◽  
Yoshiya Uwatoko
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Low Temperature ◽  
High Magnetic Field ◽  
High Pressure Apparatus

Photoluminescence spectroscopy of self-assembled InAs quantum dots in strong magnetic field and under high pressure

1997 ◽  
Vol 70 (4) ◽  
pp. 505-507 ◽  
Author(s):  
I. E. Itskevich ◽  
M. Henini ◽  
H. A. Carmona ◽  
L. Eaves ◽  
P. C. Main ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Quantum Dots ◽  
High Pressure ◽  
Strong Magnetic Field ◽  
Photoluminescence Spectroscopy ◽  
Inas Quantum Dots ◽  
Self Assembled

Electrical resistivity of single crystalline UGe2 at high pressure and high magnetic field

1995 ◽  
Vol 206-207 ◽  
pp. 515-518 ◽  
Author(s):  
Gendo Oomi ◽  
Tomoko Kagayama ◽  
Kazutaka Nishimura ◽  
S.W. Yun ◽  
Yoshichika Ōnuki
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Electrical Resistivity ◽  
High Magnetic Field ◽  
Single Crystalline

Magnetic-field and high-pressure dependences of Tc and critical current in the polycrystalline HgBaCaCuO system

1995 ◽  
Vol 251 (3-4) ◽  
pp. 207-215 ◽  
Author(s):  
A.I. D'yachenko ◽  
V.Yu. Tarenkov ◽  
A.V. Abalioshev ◽  
R.V. Lutciv ◽  
Yu.N. Myasoedov ◽  
...  
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Critical Current

Magnetic properties of synthetic taenite at high pressure

2020 ◽  
Author(s):  
Catherine McCammon ◽  
Qingguo Wei ◽  
Stuart Gilder
Keyword(s):  
Magnetic Field ◽  
High Pressure ◽  
Magnetic Properties ◽  
Nickel Alloy ◽  
Traditional Approach ◽  
Major Constituent ◽  
Open Questions ◽  
Field Fluctuations ◽  
Iron Nickel ◽  
Diamond Anvil

<p>Taenite, an iron-nickel alloy with 20-40 at% nickel, is a major constituent of iron meteorites that have been used to infer planetary core compositions. Many aspects of its magnetic properties are controversial, particularly near the Invar (“invariable”) composition around 36 at% nickel. Open questions include the conditions under which magnetism is lost, so to address this particular controversy, we undertook a combined magnetic remanence and Mössbauer study of synthetic taenite at high pressure. We synthesised polycrystalline iron-nickel alloy with 38 at% nickel, loaded the sample into a diamond anvil cell and collected Mössbauer spectra during decompression from 20 GPa. Our results show a clear loss of magnetism, but at pressures that differ considerably depending on the fitting model. The pressure obtained using the traditional approach involving a magnetic field distribution conflicts with results obtained from other methods, while a simple model based on magnetic field fluctuations gives results that are consistent with other data. Comparison of data from all methods provides insight that can be applied to planetary magnetism.</p>

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