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L. Lu

Publications and source records attributed to L. Lu.

45 records · Page 3Linked to original sources
arXiv2003

Tunneling into Multiwalled Carbon Nanotubes: Coulomb Blockade and Fano Resonance

Tunneling spectroscopy measurements of single tunnel junctions formed between multiwalled carbon nanotubes (MWNTs) and a normal metal are reported. Intrinsic Coulomb interactions in the MWNTs give rise to a strong zero-bias suppression of a tunneling density of states (TDOS) that can be fitted numerically to the environmental quantum-fluctuation (EQF) theory. An asymmetric conductance anomaly near zero bias is found at low temperatures and interpreted as Fano resonance in the strong tunneling regime.

cond-mat.mes-hall↗
arXiv2002

Order Parameter Criticality of the d=3 Random-Field Ising Antiferromagnet Fe(0.85)Zn(0.15)F2

The critical exponent beta =0.16 +- 0.02 for the random-field Ising model order parameter is determined using extinction-free magnetic x-ray scattering for Fe(0.85)Zn(0.15)F2 in magnetic fields of 10 and 11 T. The observed value is consistent with other experimental random-field critical exponents, but disagrees sharply with Monte Carlo and exact ground state calculations on finite-sized systems.

cond-mat.dis-nn↗
arXiv2002

Behavior of Sulfur Abundances in Metal-Poor Giants and Dwarfs

LTE and NLTE abundances of sulfur in 6 metal-poor giants and 61 dwarfs (62 dwarfs, including the Sun) were explored in the range of -3 \lsim [Fe/H] \lsim $+0.5$ using high-resolution, high signal-to-noise ratio spectra of the \SI 8693.9 Åand 8694.6 Ålines observed by us and measured by \Francois (1987, 1988) and Clegg et al. (1981). NLTE effects in S abundances are found to be small and practically negligible. The behavior of [S/Fe] vs. [Fe/H] exhibits a linear increasing trend without plateau with decreasing [Fe/H]. Combining our results with those available in the literature, we find that the slope of the increasing trend is -0.25 in the NLTE behavior of [S/Fe], which is comparable to that observed in [O/Fe]. The observed behavior of S may require chemical evolution models of the Galaxy, in which scenarios of hypernovae nucleosynthesis and/or time-delayed deposition into interstellar medium are incorporated.

astro-ph↗
arXiv2002

Observation of room-temperature spontaneous phase segregation in overdoped Bi$_2$Sr$_2$CaCu$_2$O$_{8+x}

The occurrence and development of phase inhomogeneity in {\rm Bi$_2$Sr$_2$CaCu$_2$O$_{8+x}$} single crystals have been investigated by measuring their superconducting transition patterns using a high-sensitivity ac magnetometer. We find that the overdoped {\rm Bi$_2$Sr$_2$CaCu$_2$O$_{8+x}$} single crystals, even if they were single-phased immediately after a high-temperature annealing process, show progressively pronounced multiple superconducting transitions with time as they were kept at room temperature in a dry air atmosphere. The results reveal that the oxygen dopants in the crystal are still mobile at room temperature. These dopants tend to re-arrange and thus form different phases, at a characteristic time scale of one or two weeks or so. Moreover, the diamagnetization loops in the newly segregated phase are very weak, presumably due to the existence of additional inhomogeneity down to a nanometer scale. Our results also show that the optimally doped {\rm Bi$_2$Sr$_2$CaCu$_2$O$_{8+x}$} crystals seem capable to remain in a single phase with time.

cond-mat.supr-con↗
arXiv2002

3 omega method for specific heat and thermal conductivity measurements

We present a 3 omega method for simultaneously measuring the specific heat and thermal conductivity of a rod- or filament-like specimen using a way similar to a four-probe resistance measurement. The specimen in this method needs to be electrically conductive and with a temperature-dependent resistance, for acting both as a heater to create a temperature fluctuation and as a sensor to measure its thermal response. With this method we have successfully measured the specific heat and thermal conductivity of platinum wire specimens at cryogenic temperatures, and measured those thermal quantities of tiny carbon nanotube bundles some of which are only 10^-9 g in mass.

quant-ph↗
arXiv2001

Preparation and Characterization of Homogeneous YBCO Single Crystals with Doping Level near the SC-AFM Boundary

High-purity and homogeneous YBa2Cu3Oy single crystals with carrier doping level near the AFM-SC boundary have been obtained in the oxygen content range between y = 6.340 and 6.370. The crystals are ortho-II phase at room temperature and undergo the orthorhombic to tetragonal transition at about 140_Degree_C. They show sharp superconducting transitions, with Tc between 4 and 20 K. Tc changes by 0.8 K when the oxygen content y is changed by 0.001, and is also sensitive to annealing conditions near room temperature, due to the dependence of doping on oxygen ordering correlation lengths. Crystals with oxygen content y lower than 6.345 are non-superconducting.

cond-mat.supr-con↗
arXiv2000

Oxygen Abundance Determination in Very Metal-Deficient Giants: Permitted O I Lines Versus Forbidden [O I] Lines

The abundance of oxygen was determined for selected very metal-poor G-K stars (six giants and one turn-off star) based on the high S/N and high-resolution spectra observed with Keck HIRES in the red through near-IR region comprising the permitted O I lines (7771-5, 8446) along with the [O I] forbidden line at 6363 A. It turned out that both the abundances from the permitted line features, O I 7771-5 and O I 8446, agree quite well with each other, while the forbidden line yields somewhat discrepant and divergent abundances with a tendency of being underestimated on the average. The former (7773/8446) solution, which we believe to be more reliable, gives a fairly tight [O/Fe] vs. [Fe/H] relation such that increasing steadily from [O/Fe] = 0.6 (at [Fe/H] = -1.5) to [O/Fe] = 1.0 (at [Fe/H] = -3.0), in reasonable consistency with the trend recently reported based on the analysis of the UV OH lines. We would suspect that some kind of weakening mechanism may occasionally act on the formation of [O I] forbidden lines in metal-poor stars. Therefore, [O I] lines may not be so a reliable abundance indicator as has been generally believed.

astro-ph↗
arXiv1997

High Signal-to-Noise GHRS Observations of H 1821+643: O VI Associated with a Group of Galaxies at z = 0.226 and Complex Lyman $α$ Absorption Profiles at Low Redshift

As part of a program to study the relationship between QSO Lyman alpha clouds and galaxies at low redshifts, we have obtained a high signal-to-noise far UV spectrum of H 1821+643 [z(em) = 0.297] with the G140L grating of the GHRS. The spectrum, which has a resolution of FWHM = 150 km/s and S/N ~ 100:1, is adequate for detection of weak Ly alpha clouds with equivalent width as low as 50 mA (4sigma) with complete spectral coverage from z_(abs) = 0.03 to z(abs) = 0.26. In this paper we present some preliminary results of this study including the following. (1) The absorption profiles of three out of the four strongest extragalactic Ly alpha lines show complex component structure with a main strong component and several weaker outlying components spanning a full velocity range of ~1000-1500 km/s. The two-point correlation function does not show any evidence of Ly alpha cloud clustering but suffers from small number statistics. (2) Extragalactic O VI is clearly detected in the intervening absorption system at z_(abs) = 0.225. Two galaxies at z = 0.2256 and z = 0.2263 are close to the sight line (the closer galaxy is at a projected distance of ~90 kpc), so this O VI absorption could be due to the intracluster medium of a group of galaxies.

astro-ph↗