5,026 research outputs found

    Thermally activated escape rates of uniaxial spin systems with transverse field

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    Classical escape rates of uniaxial spin systems are characterized by a prefactor differing from and much smaller than that of the particle problem, since the maximum of the spin energy is attained everywhere on the line of constant latitude: theta=const, 0 =< phi =< 2*pi. If a transverse field is applied, a saddle point of the energy is formed, and high, moderate, and low damping regimes (similar to those for particles) appear. Here we present the first analytical and numerical study of crossovers between the uniaxial and other regimes for spin systems. It is shown that there is one HD-Uniaxial crossover, whereas at low damping the uniaxial and LD regimes are separated by two crossovers.Comment: 4 PR pages, 3 figures, final published versio

    Field dependence of the temperature at the peak of the ZFC magnetization

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    The effect of an applied magnetic field on the temperature at the maximum of the ZFC magnetization, MZFCM_{ZFC}, is studied using the recently obtained analytic results of Coffey et al. (Phys. Rev. Lett. {\bf 80}(1998) 5655) for the prefactor of the N\'{e}el relaxation time which allow one to precisely calculate the prefactor in the N\'{e}el-Brown model and thus the blocking temperature as a function of the coefficients of the Taylor series expansion of the magnetocrystalline anisotropy. The present calculations indicate that even a precise determination of the prefactor in the N\'{e}el-Brown theory, which always predicts a monotonic decrease of the relaxation time with increasing field, is insufficient to explain the effect of an applied magnetic field on the temperature at the maximum of the ZFC magnetization. On the other hand, we find that the non linear field-dependence of the magnetization along with the magnetocrystalline anisotropy appears to be of crucial importance to the existence of this maximum.Comment: 14 LaTex209 pages, 6 EPS figures. To appear in J. Phys.: Condensed Matte

    Magnetic susceptibility of a CuO2 plane in the La2CuO4 system: I. RPA treatment of the Dzyaloshinskii-Moriya Interactions

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    Motivated by recent experiments on undoped La2CuO4, which found pronounced temperature-dependent anisotropies in the low-field magnetic susceptibility, we have investigated a two-dimensional square lattice of S=1/2 spins that interact via Heisenberg exchange plus the symmetric and anti-symmetric Dzyaloshinskii-Moriya anisotropies. We describe the transition to a state with long-ranged order, and find the spin-wave excitations, with a mean-field theory, linear spin-wave analysis, and using Tyablikov's RPA decoupling scheme. We find the different components of the susceptibility within all of these approximations, both below and above the N'eel temperature, and obtain evidence of strong quantum fluctuations and spin-wave interactions in a broad temperature region near the transition.Comment: 20 pages, 2 column format, 22 figure

    Quantum Thermoactivation of Nanoscale Magnets

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    The integral relaxation time describing the thermoactivated escape of a uniaxial quantum spin system interacting with a boson bath is calculated analytically in the whole temperature range. For temperatures T much less than the barrier height \Delta U, the level quantization near the top of the barrier and the strong frequency dependence of the one-boson transition probability can lead to the regularly spaced deep minima of the thermoactivation rate as a function of the magnetic field applied along the z axis.Comment: 4 pages, no figures, rejected from Phys. Rev. Let

    Integral Relaxation Time of Single-Domain Ferromagnetic Particles

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    The integral relaxation time \tau_{int} of thermoactivating noninteracting single-domain ferromagnetic particles is calculated analytically in the geometry with a magnetic field H applied parallel to the easy axis. It is shown that the drastic deviation of \tau_{int}^{-1} from the lowest eigenvalue of the Fokker-Planck equation \Lambda_1 at low temperatures, starting from some critical value of H, is the consequence of the depletion of the upper potential well. In these conditions the integral relaxation time consists of two competing contributions corresponding to the overbarrier and intrawell relaxation processes.Comment: 8 pages, 3 figure

    Organic molecules in the protoplanetary disk of DG Tau revealed by ALMA

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    Planets form in protoplanetary disks and inherit their chemical compositions. It is thus crucial to map the distribution and investigate the formation of simple organics, such as formaldehyde and methanol, in protoplanetary disks. We analyze ALMA observations of the nearby disk-jet system around the T Tauri star DG Tau in the o-H2_2CO 31,221,13_{1,2}-2_{1,1} and CH3_3OH 32,241,43_{-2,2}-4_{-1,4} E, 50,540,45_{0,5}-4_{0,4} A transitions at an unprecedented resolution of 0.15"\sim0.15", i.e., 18\sim18 au at a distance of 121 pc. The H2_2CO emission originates from a rotating ring extending from 40\sim40 au with a peak at 62\sim62 au, i.e., at the edge of the 1.3mm dust continuum. CH3_3OH emission is not detected down to an r.m.s. of 3 mJy/beam in the 0.162 km/s channel. Assuming an ortho-to-para ratio of 1.8-2.8 the ring- and disk-height-averaged H2_2CO column density is 0.34×1014\sim0.3-4\times10^{14} cm2^{-2}, while that of CH3_3OH is <0.040.7×1014<0.04-0.7\times10^{14} cm2^{-2}. In the inner 4040 au no o-H2_2CO emission is detected with an upper limit on its beam-averaged column density of 0.56×1013\sim0.5-6\times10^{13} cm2^{-2}. The H2_2CO ring in the disk of DG Tau is located beyond the CO iceline (RCO30_{\rm CO}\sim30 au). This suggests that the H2_2CO abundance is enhanced in the outer disk due to formation on grain surfaces by the hydrogenation of CO ice. The emission peak at the edge of the mm dust continuum may be due to enhanced desorption of H2_2CO in the gas phase caused by increased UV penetration and/or temperature inversion. The CH3_3OH/H2_2CO abundance ratio is <1<1, in agreement with disk chemistry models. The inner edge of the H2_2CO ring coincides with the radius where the polarization of the dust continuum changes orientation, hinting at a tight link between the H2_2CO chemistry and the dust properties in the outer disk and at the possible presence of substructures in the dust distribution.Comment: 8 pages, 6 figures, accepted for publication on A&A Letter

    Accurate Results from Perturbation Theory for Strongly Frustrated S=1/2S=1/2 Heisenberg Spin Clusters

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    We investigate the use of perturbation theory in finite sized frustrated spin systems by calculating the effect of quantum fluctuations on coherent states derived from the classical ground state. We first calculate the ground and first excited state wavefunctions as a function of applied field for a 12-site system and compare with the results of exact diagonalization. We then apply the technique to a 20-site system with the same three fold site coordination as the 12-site system. Frustration results in asymptotically convergent series for both systems which are summed with Pad\'e approximants. We find that at zero magnetic field the different connectivity of the two systems leads to a triplet first excited state in the 12-site system and a singlet first excited state in the 20-site system, while the ground state is a singlet for both. We also show how the analytic structure of the Pad\'e approximants at λ1|\lambda| \simeq 1 evolves in the complex λ\lambda plane at the values of the applied field where the ground state switches between spin sectors and how this is connected with the non-trivial dependence of the number on the strength of quantum fluctuations. We discuss the origin of this difference in the energy spectra and in the analytic structures. We also characterize the ground and first excited states according to the values of the various spin correlation functions.Comment: Final version, accepted for publication in Physical review

    Adiabatic and Non-Adiabatic Contributions to the Free Energy from the Electron-Phonon Interaction for Na, K, Al, and Pb

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    We calculate the adiabatic contributions to the free energy due to the electron--phonon interaction at intermediate temperatures, 0kBT<ϵF0 \leqslant k_{B} T < \epsilon_{F} for the elemental metals Na, K, Al, and Pb. Using our previously published results for the nonadiabatic contributions we show that the adiabatic contribution, which is proportional to T2T^{2} at low temperatures and goes as T3T^{3} at high temperatures, dominates the nonadiabatic contribution for temperatures above a cross--over temperature, TcT_{c}, which is between 0.5 and 0.8 TmT_{m}, where TmT_{m} is the melting temperature of the metal. The nonadiabatic contribution falls as T1T^{-1} for temperatures roughly above the average phonon frequency.Comment: Updated versio

    Monte Carlo simulation with time step quantification in terms of Langevin dynamics

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    For the description of thermally activated dynamics in systems of classical magnetic moments numerical methods are desirable. We consider a simple model for isolated magnetic particles in a uniform field with an oblique angle to the easy axis of the particles. For this model, a comparison of the Monte Carlo method with Langevin dynamics yields new insight in the interpretation of the Monte Carlo process, leading to the implementation of a new algorithm where the Monte Carlo step is time-quantified. The numeric results for the characteristic time of the magnetisation reversal are in excellent agreement with asymptotic solutions which itself are in agreement with the exact numerical results obtained from the Fokker-Planck equation for the Neel-Brown model.Comment: 5 pages, Revtex, 4 Figures include

    A bulk 2D Pauli Limited Superconductor

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    We present a nearly perfect Pauli-limited critical field phase diagram for the anisotropic organic superconductor \α\alpha-(ET)2_2NH4_4(SCN)4_4 when the applied magnetic field is oriented parallel to the conducting layers. The critical fields ({H_{c_2}) were found by use of penetration depth measurements. Because {H_{c_2} is Pauli-limited, the size of the superconducting energy gap can be calculated. The role of spin-orbit scattering and many-body effects play a role in explaining our measurements.Comment: 4 pages, 5 figures. V5, corrections were made to the text, present data was include
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