4,231 research outputs found

    Kosterlitz-Thouless Phase Transition of the ANNNI model in Two Dimensions

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    The spin structure of an axial next-nearest-neighbor Ising (ANNNI) model in two dimensions (2D) is a renewed problem because different Monte Carlo (MC) simulation methods predicted different spin orderings. The usual equilibrium simulation predicts the occurrence of a floating incommensurate (IC) Kosterlitz-Thouless (KT) type phase, which never emerges in non-equilibrium relaxation (NER) simulations. In this paper, we first examine previously published results of both methods, and then investigate a higher transition temperature, Tc1T_{c1}, between the IC and paramagnetic phases. In the usual equilibrium simulation, we calculate the layer magnetization on larger lattices (up to 512×512512 \times 512 sites) and estimate Tc1≈1.16JT_{c1} \approx 1.16J with frustration ratio κ(≡−J2/J1)=0.6\kappa (\equiv -J_2/J_1) = 0.6. We examine the nature of the phase transition in terms of the Binder ratio gLg_L of spin overlap functions and the correlation-length ratio ξ/L\xi/L. In the NER simulation, we observe the spin dynamics in equilibrium states by means of an autocorrelation function, and also observe the layer magnetization relaxations from the ground and disordered states. These quantities exhibit an algebraic decay at T≲1.17JT \lesssim 1.17J. We conclude that the two-dimensional ANNNI model actually admits an IC phase transition of the KT type.Comment: 20 pages, 16 figure

    An improved method for determining the DC magnetization curve using a ring specimen

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    When the DC magnetization curve (B-H) of nonoriented material is measured in a ring specimen, there is an intrinsic error due to the assumption that the mean magnetic path length is equal to the mean geometric path length. A novel method for determining the B-H curve accurately is proposed. The validity of the method is verified by experiments</p

    Attracting shallow donors: Hydrogen passivation in (Al,Ga,In)-doped ZnO

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    The hydrogen interstitial and the substitutional Al_Zn, Ga_Zn and In_Zn are all shallow donors in ZnO and lead to n-type conductivity. Although shallow donors are expected to repel each other, we show by first principles calculations that in ZnO these shallow donor impurities attract and form a complex, leading to a donor level deep in the band gap. This puts a limit on the n-type conductivity of (Al,Ga,In)-doped ZnO in the presence of hydrogen.Comment: 4 pages, 5 figure

    Spin-Glass and Chiral-Glass Transitions in a ±J\pm J Heisenberg Spin-Glass Model in Three Dimensions

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    The three-dimensional ±J\pm J Heisenberg spin-glass model is investigated by the non-equilibrium relaxation method from the paramagnetic state. Finite-size effects in the non-equilibrium relaxation are analyzed, and the relaxation functions of the spin-glass susceptibility and the chiral-glass susceptibility in the infinite-size system are obtained. The finite-time scaling analysis gives the spin-glass transition at Tsg/J=0.21−0.02+0.01T_{\rm sg}/J=0.21_{-0.02}^{+0.01} and the chiral-glass transition at Tcg/J=0.22−0.03+0.01T_{\rm cg}/J=0.22_{-0.03}^{+0.01}. The results suggest that both transitions occur simultaneously. The critical exponent of the spin-glass susceptibility is estimated as γsg=1.7±0.3\gamma_{\rm sg}= 1.7 \pm 0.3, which makes an agreement with the experiments of the insulating and the canonical spin-glass materials.Comment: 4 pages, 2 figure

    Magneto-optics induced by the spin chirality in itinerant ferromagnet Nd2_2Mo2_2O7_7

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    It is demonstrated both theoretically and experimentally that the spin chirality associated with a noncoplanar spin configuration produces a magneto-optical effect. Numerical study of the two-band Hubbard model on a triangle cluster shows that the optical Hall conductivity σxy(ω)\sigma_{xy}(\omega) is proportional to the spin chirality. The detailed comparative experiments on pyrochlore-type molybdates R2R_2Mo2_2O7_7 with R=R=Nd (Ising-like moments) and R=R=Gd (Heisenberg-like ones) clearly distinguishes the two mechanisms, i.e., spin chirality and spin-orbit interactions. It is concluded that for RR=Nd, σxy(ω)\sigma_{xy}(\omega) is dominated by the spin chirality for the dc (ω=0\omega=0) and the d→dd \to d incoherent intraband optical transitions between Mo atoms.Comment: 4 pages, 5 figures. submitted to Phys. Rev.

    Search for weak M1 transitions in 48^{48}Ca with inelastic proton scattering

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    The spinflip M1 resonance in the doubly magic nucleus 48^{48}Ca, dominated by a single transition, serves as a reference case for the quenching of spin-isospin modes in nuclei. The aim of the present work is a search for weak M1 transitions in 48^{48}Ca with a high-resolution (p,p') experiment at 295 MeV and forward angles including 0 degree and a comparison to results from a similar study using backward-angle electron scattering at low momentum transfers in order to estimate their contribution to the total B(M1) strength. M1 cross sections of individual peaks in the spectra are deduced with a multipole decomposition analysis. The corresponding reduced B(M1) transition strengths are extracted following the approach outlined in J. Birkhan et al., Phys. Rev. C 93, 041302(R) (2016). In total, 29 peaks containing a M1 contribution are found in the excitation energy region 7 - 13 MeV. The resulting B(M1) strength distribution compares well to the electron scattering results considering different factors limiting the sensitivity in both experiments and the enhanced importance of mechanisms breaking the proportionality of nuclear cross sections and electromagnetic matrix elements for weak transitions as studied here. The total strength of 1.19(6) μN2\mu_N^2 deduced assuming a non-quenched isoscalar part of the (p,p') cross sections agrees with the (e,e') result of 1.21(13) μN2\mu_N^2. A binwise analysis above 10 MeV provides an upper limit of 1.62(23) μN2\mu_N^2. The present results confirm that weak transitions contribute about 25% to the total B(M1) strength in 48^{48}Ca and the quenching factors of GT and spin-M1 strength are comparable in fp-shell nuclei. Thus, the role of of meson exchange currents seems to be neglible, in contrast to sd-shell nuclei.Comment: 11 pages, 9 figures, revised analysis with oxygen contamination remove

    Measurement of energy muons in EAS at energy region larger thean 10(17) eV

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    A measurement of low energy muons in extensive air showers (EAS) (threshold energies are 0.25, 0.5, 0.75 and 1.38 GeV) was carried out. The density under the concrete shielding equivalent to 0.25 GeV at core distance less than 500 m and 0.5 GeV less than 150 m suffers contamination of electromagnetic components. Therefore the thickness of concrete shielding for muon detectors for the giant air shower array is determined to be 0.5 GeV equivalence. Effects of photoproduced muons are found to be negligible in the examined ranges of shower sizes and core distances. The fluctuation of the muon density in 90 sq m is at most 25% between 200 m and 600 m from the core around 10 to the 17th power eV

    Redshift-space Distortions of the Power Spectrum of Cosmological Objects on a Light Cone : Explicit Formulations and Theoretical Implications

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    We examine the effects of the linear and the cosmological redshift-space distortions on the power spectrum of cosmological objects on a light cone. We develop theoretical formulae for the power spectrum in linear theory of density perturbations in a rigorous manner starting from first principle corresponding to Fourier analysis. Approximate formulae, which are useful properly to incorporate the redshift-space distortion effects into the power spectrum are derived, and the validity is examined. Applying our formulae to galaxy and quasar samples which roughly match the SDSS survey, we will show how the redshift-space distortions distort the power spectrum on the light cone quantitatively.Comment: 30 pages, Accepted for publication in the Astrophysical Journal Supplement Serie

    Magnetic Excitations in the Quasi-1D Ising-like Antiferromagnet TlCoCl3_3

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    Neutron inelastic scattering measurements have been performed in order to investigate the magnetic excitations in the quasi-1D Ising-like antiferromagnet TlCoCl3_3. We observed the magnetic excitation, which corresponds to the spin-wave excitation continuum corresponding to the domain-wall pair excitation in the 1D Ising-like antiferromagnet. According to the Ishimura-Shiba theory, we analyzed the observed spin-wave excitation, and the exchange constant 2J2J and the anistropy ϵ\epsilon were estimated as 14.7 meV and 0.14 in TlCoCl3_3, respectively.Comment: 2 pages, 3 figures, jpsj2.cls, to be published in J. Phys. Soc. Jpn. Vol.75 (2006) No.

    Scaling Theory of Antiferromagnetic Heisenberg Ladder Models

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    The S=1/2S=1/2 antiferromagnetic Heisenberg model on multi-leg ladders is investigated. Criticality of the ground-state transition is explored by means of finite-size scaling. The ladders with an even number of legs and those with an odd number of legs are distinguished clearly. In the former, the energy gap opens up as ΔE∼J⊥\Delta E\sim{J_\perp}, where J⊥{J_\perp} is the strength of the antiferromagnetic inter-chain coupling. In the latter, the critical phase with the central charge c=1c=1 extends over the whole region of J⊥>0{J_\perp}>0.Comment: 12 pages with 9 Postscript figures. To appear in J. Phys. A: Math. Ge
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