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Dive into the research topics where X.L. Yan is active.

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Featured researches published by X.L. Yan.


The Astrophysical Journal | 2013

Mass Measurement of 45Cr and Its Impact on the Ca-Sc Cycle in X-Ray Bursts

X.L. Yan; H. Xu; Yu. A. Litvinov; Yueyang Zhang; H. Schatz; X. L. Tu; Klaus Blaum; X. H. Zhou; B. Sun; J. He; Yang Sun; Meng Wang; Y. Yuan; J.W. Xia; J. Yang; G. Audi; G. B. Jia; Z. G. Hu; X. W. Ma; R. S. Mao; B. Mei; P. Shuai; Z. Y. Sun; S. T. Wang; Guoqing Xiao; X. Xu; Takayuki Yamaguchi; Y. Yamaguchi; Y. D. Zang; H. Zhao

Masses of neutron-deficient 58Ni projectile fragments have been measured at the HIRFL-CSR facility in Lanzhou, China employing the isochronous mass spectrometry technique. Masses of a series of short-lived Tz = –3/2 nuclides including the 45Cr nucleus have been measured with a relative uncertainty of about 10–6-10–7. The new 45Cr mass turned out to be essential for modeling the astrophysical rp-process. In particular, we find that the formation of the predicted Ca-Sc cycle in X-ray bursts can be excluded.


Physical Review Letters | 2011

Electronic Structures and Magnetic Order of Ordered-Fe-Vacancy Ternary Iron Selenides TlFe1.5Se2 and AFe(1.5)Se(2) (A = K, Rb, or Cs)

X.L. Yan; Miao Gao; Zhong-Yi Lu; Tao Xiang

By the first-principles electronic structure calculations, we find that the ground state of the Fe-vacancies ordered TlFe1.5Se2 is a quasi-two-dimensional collinear antiferromagnetic semiconductor with an energy gap of 94 meV, in agreement with experimental measurements. This antiferromagnetic order is driven by the Se-bridged antiferromagnetic superexchange interactions between Fe moments. Similarly, we find that crystals AFe(1.5)Se(2) (A = K, Rb, or Cs) are also antiferromagnetic semiconductors but with a zero-gap semiconducting state or semimetallic state nearly degenerated with the ground states. Thus, rich physical properties and phase diagrams are expected.


Physics Letters B | 2013

High-resolution measurement of the time-modulated orbital electron capture and of the β+ decay of hydrogen-like 142Pm60+ ions

P. Kienle; F. Bosch; P. Bühler; T. Faestermann; Yu. A. Litvinov; N. Winckler; M. S. Sanjari; Daria Shubina; Dinko Atanasov; H. Geissel; V. Ivanova; X.L. Yan; D. Boutin; C. Brandau; I. Dillmann; Ch. Dimopoulou; R Hess; P.-M. Hillebrand; T. Izumikawa; R. Knöbel; J. Kurcewicz; N. Kuzminchuk; M. Lestinsky; S. Litvinov; X. W. Ma; L. Maier; M. Mazzocco; I. Mukha; C. Nociforo; F. Nolden

Abstract The periodic time modulations, found recently in the two-body orbital electron capture (EC) decay of both, hydrogen-like 140Pr58+ and 142Pm60+ ions, with periods near to 7 s and amplitudes of about 20%, were re-investigated for the case of 142Pm60+ by using a 245 MHz resonator cavity with a much improved sensitivity and time resolution. We observed that the exponential EC decay is modulated with a period T = 7.11 ( 11 ) s , in accordance with a modulation period T = 7.12 ( 11 ) s as obtained from simultaneous observations with a capacitive pick-up, employed also in the previous experiments. The modulation amplitudes amount to a R = 0.107 ( 24 ) and a P = 0.134 ( 27 ) for the 245 MHz resonator and the capacitive pick-up, respectively. These new results corroborate for both detectors exactly our previous findings of modulation periods near to 7 s , though with distinctly smaller amplitudes. Also the three-body β + decays have been analyzed. For a supposed modulation period near to 7 s we found an amplitude a = 0.027 ( 27 ) , compatible with a = 0 and in agreement with the preliminary result a = 0.030 ( 30 ) of our previous experiment. These observations could point at weak interaction as origin of the observed 7 s -modulation of the EC decay. Furthermore, the data suggest that interference terms occur in the two-body EC decay, although the neutrinos are not directly observed.


Physical Review B | 2011

Electronic and magnetic structures of the ternary iron selenides AFe(2)Se(2) ( A = Cs, Rb, K, or Tl)

X.L. Yan; Miao Gao; Zhong-Yi Lu; Tao Xiang

We have studied the electronic and magnetic structures of the ternary iron selenides AFe(2)Se(2) (A = Cs, Rb, K, or Tl) using first-principles electronic structure calculations. We find that the ground state of these compounds is bicollinearly antiferromagnetically ordered, with the Fe moments having collinear antiferromagnetic order in each bipartite sublattice. This bicollinear antiferromagnetic order results from the superexchange interactions of Fe moments mediated by the Se 4p orbitals. We have also determined the density of states at the Fermi level, the specific heat coefficient, the Pauli susceptibility, and other related physical properties in both the nonmagnetic and bicollinear antiferromagnetic states for these compounds. The underlying mechanism is discussed according to the electronic structure analysis.


Physical Review B | 2011

Ternary iron selenideK0.8Fe1.6Se2is an antiferromagnetic semiconductor

X.L. Yan; Miao Gao; Zhong-Yi Lu; Tao Xiang

We have studied electronic and magnetic structures of K0.8+xFe1.6Se2 by performing the first-principles electronic structure calculations. The ground state of the Fe-vacancies ordered K0.8Fe1.6Se2 is found to be a quasi-two-dimensional blocked checkerboard antiferromagnetic (AFM) semiconductor with an energy gap of 594 meV and a large ordering magnetic moment of 3.37 mu B for each Fe atom, in excellent agreement with the neutron-scattering measurement. The underlying mechanism is the chemical-bonding-driven tetramer lattice distortion. K0.8+xFe1.6Se2 with finite x is a doped AFM semiconductor with low conducting carrier concentration, which is approximately proportional to the excess potassium content, consistent qualitatively with the infrared observation. Our study reveals the importance of the interplay between antiferromagnetism and superconductivity in these materials. This suggests that K0.8Fe1.6Se2, instead of KFe2Se2, should be regarded as a parent compound from which the superconductivity emerges upon electron or hole doping.


Astrophysical Journal Supplement Series | 2015

THE FORMATION AND MAGNETIC STRUCTURES OF ACTIVE-REGION FILAMENTS OBSERVED BY NVST, SDO, AND HINODE

X.L. Yan; Z. K. Xue; G. M. Pan; Jiancheng Wang; Yongyuan Xiang; D. F. Kong; Liheng Yang

To better understand the properties of solar active-region filaments, we present a detailed study on the formation and magnetic structures of two active-region filaments in active region NOAA 11884 during a period of four days. It is found that the shearing motion of the opposite magnetic polarities and the rotation of the small sunspots with negative polarity play an important role in the formation of two active-region filaments. During the formation of these two active-region filaments, one foot of the filaments was rooted in a small sunspot with negative polarity. The small sunspot rotated not only around another small sunspot with negative polarity, but also around the center of its umbra. By analyzing the nonlinear force-free field extrapolation using the vector magnetic fields in the photosphere, twisted structures were found in the two active-region filaments prior to their eruptions. These results imply that the magnetic fields were dragged by the shearing motion between opposite magnetic polarities and became more horizontal. The sunspot rotation twisted the horizontal magnetic fields and finally formed the twisted active-region filaments.


Physical Review Letters | 2016

Identification of the Lowest T =2, Jπ =0+ Isobaric Analog State in 52Co and Its Impact on the Understanding of β-Decay Properties of52Ni

X. Xu; Pengjie Zhang; P. Shuai; R.J. Chen; X.L. Yan; Y. H. Zhang; M. Wang; Yu. A. Litvinov; H. Xu; T. Bao; X. Chen; H. S. Chen; C. Y. Fu; Shigeru Kubono; Y. H. Lam; Dean Liu; R. S. Mao; X. W. Ma; M. Z. Sun; X. L. Tu; Y. M. Xing; J. Yang; Y. Yuan; Qin Zeng; X. J. Zhou; X. H. Zhou; W. L. Zhan; S. Litvinov; Klaus Blaum; G. Audi

Masses of ^{52g,52m}Co were measured for the first time with an accuracy of ∼10  keV, an unprecedented precision reached for short-lived nuclei in the isochronous mass spectrometry. Combining our results with the previous β-γ measurements of ^{52}Ni, the T=2, J^{π}=0^{+} isobaric analog state (IAS) in ^{52}Co was newly assigned, questioning the conventional identification of IASs from the β-delayed proton emissions. Using our energy of the IAS in ^{52}Co, the masses of the T=2 multiplet fit well into the isobaric multiplet mass equation. We find that the IAS in ^{52}Co decays predominantly via γ transitions while the proton emission is negligibly small. According to our large-scale shell model calculations, this phenomenon has been interpreted to be due to very low isospin mixing in the IAS.


The Astrophysical Journal | 2016

THE FORMATION OF AN INVERSE S-SHAPED ACTIVE-REGION FILAMENT DRIVEN BY SUNSPOT MOTION AND MAGNETIC RECONNECTION

X.L. Yan; E. R. Priest; Q. L. Guo; Z. K. Xue; Jiancheng Wang; Liheng Yang

We present a detailed study of the formation of an inverse S-shaped filament prior to its eruption in active region NOAA 11884 from October 31 to November 2, 2013. In the initial stage, clockwise rotation of a small positive sunspot around the main negative trailing sunspot formed a curved filament. Then the small sunspot cancelled with negative magnetic flux to create a longer active-region filament with an inverse S-shape. At the cancellation site a brightening was observed in UV and EUV images and bright material was transferred to the filament. Later the filament erupted after cancellation of two opposite polarities under the upper part of the filament. Nonlinear force-free field (NLFFF) extrapolation of vector photospheric fields suggests that the filament may have a twisted structure, but this cannot be confirmed from the current observations.


Physica Scripta | 2013

Half-life measurements of highly charged radionuclides

Dinko Atanasov; D. L. Balabanski; L. Batist; Klaus Blaum; F. Bosch; D. Boutin; C. Brandau; C. Dimopoulou; H G Essel; T. Faestermann; H. Geissel; S. Hagmann; R Hess; P.-M. Hillenbrand; P. Kienle; R. Knöbel; C. Kozhuharov; J. Kurcewicz; M. Lestinsky; S. Litvinov; Yu. A. Litvinov; X. W. Ma; R Märtin; M. Mazzocco; G. Münzenberg; F. Nolden; T. Ohtsubo; Z. Patyk; M. S. Sanjari; C. Scheidenberger

In recent years several measurements of the orbital electron capture half-lives of few-electron ions have been carried out employing the storage ring ESR at GSI. Hydrogen-like and helium-like 140Pr and 142Pm as well as hydrogen-like 122I were studied. Half-lives of the corresponding fully ionized nuclides provide the three-body β+ decay constants.


Nuclear Instruments & Methods in Physics Research Section B-beam Interactions With Materials and Atoms | 2016

An improvement of isochronous mass spectrometry: Velocity measurements using two time-of-flight detectors

P. Shuai; X. Xu; Y. H. Zhang; Hu-Shan Xu; Yuri A. Litvinov; M. Wang; X. L. Tu; Klaus Blaum; X. H. Zhou; Y. Yuan; X.L. Yan; X.C. Chen; R.J. Chen; C. Y. Fu; Z. Ge; W.J. Huang; Y. M. Xing; Qin Zeng

Abstract Isochronous mass spectrometry (IMS) in storage rings is a powerful tool for mass measurements of exotic nuclei with very short half-lives down to several tens of microseconds, using a multicomponent secondary beam separated in-flight without cooling. However, the inevitable momentum spread of secondary ions limits the precision of nuclear masses determined by using IMS. Therefore, the momentum measurement in addition to the revolution period of stored ions is crucial to reduce the influence of the momentum spread on the standard deviation of the revolution period, which would lead to a much improved mass resolving power of IMS. One of the proposals to upgrade IMS is that the velocity of secondary ions could be directly measured by using two time-of-flight (double TOF) detectors installed in a straight section of a storage ring. In this paper, we outline the principle of IMS with double TOF detectors and the method to correct the momentum spread of stored ions.

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Y. H. Zhang

Chinese Academy of Sciences

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P. Shuai

Chinese Academy of Sciences

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X. L. Tu

Chinese Academy of Sciences

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X. W. Ma

Chinese Academy of Sciences

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X. Xu

Chinese Academy of Sciences

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X. H. Zhou

Chinese Academy of Sciences

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Y. Yuan

Nanyang Technological University

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R. S. Mao

Chinese Academy of Sciences

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Yu. A. Litvinov

Goethe University Frankfurt

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