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相关论文: Relativistic Effects on X-ray Structure Factors

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Halogen bond (X-bond) is a noncovalent interaction between a halogen atom and an electron donor. It is often rationalized by a region of the positive electrostatic potential on the halogen atom, so-called $\sigma$-hole. The X-bond strength…

化学物理 · 物理学 2020-06-04 Michal H. Kolář , Denisa Suchá , Michal Pitoňák

We derive the exact analytical solution of the linear structure growth rate in LCDM cosmology with flat or curved geometry, under the Newtonian gauge. Unlike the well known solution under the Newtonian limit (Heath 1977), our solution takes…

宇宙学与河外天体物理 · 物理学 2011-03-22 Pengjie Zhang

The variational method, within the Hamiltonian formalism of reformulated QED is used to determine relativistic wave equations for a system of three fermions of arbitrary mass interacting electromagnetically. The interaction kernels of the…

原子物理 · 物理学 2007-06-21 Mark Barham , Jurij W. Darewych

The kagome Hubbard model (KHM) is a paradigmatic example of a frustrated two-dimensional model. While its strongly correlated regime, described by a Heisenberg model, is of topical interest due to its enigmatic prospective spin-liquid…

强关联电子 · 物理学 2021-11-04 Josef Kaufmann , Klaus Steiner , Richard T. Scalettar , Karsten Held , Oleg Janson

We investigate roles of electron correlation effects in the determination of the $g_j$ factors of the $4s ~ ^2S_{1/2}$, $4p ~ ^2P_{1/2}$, $4p ~ ^2P_{3/2}$, $3d ~ ^2D_{3/2}$, and $3d ~ ^2D_{5/2}$ states, representing to different parities…

原子物理 · 物理学 2017-07-26 B. K. Sahoo , Pradeep Kumar

Feedback processes from baryons are expected to strongly affect weak-lensing observables of current and future cosmological surveys. In this paper we present a new parametrisation of halo profiles based on gas, stellar, and dark matter…

We extend our relativistic theory of electroweak properties of composite systems to describe simultaneously the gravitational form factors of hadrons. The approach is based on a version of the instant-form relativistic quantum mechanics and…

高能物理 - 唯象学 · 物理学 2021-02-04 A. F. Krutov , V. E. Troitsky

We demonstrate that a relativistic constituent-quark model can give nucleon form factors in agreement with data for both low and high momentum transfer. The relativistic features of the model and the specific form of the wave function are…

高能物理 - 唯象学 · 物理学 2009-10-22 Felix Schlumpf

The study of relativistic, higher order and nonlinear effects has become necessary in recent years in the pursuit of precision cosmology. We develop and apply here a framework to study gravitational lensing in exact models in general…

宇宙学与河外天体物理 · 物理学 2015-06-18 M. A. Troxel , Mustapha Ishak , Austin Peel

The nonlinear optical properties and electro-optic effects of some oxygen-octahedric ferroelectrics are studied by the density functional theory (DFT) in the local density approximation (LDA) expressions based on first principle…

材料科学 · 物理学 2011-12-30 Amirullah M. Mamedov , Ekmel Ozbay

Future surveys will access large volumes of space and hence very long wavelength fluctuations of the matter density and gravitational field. It has been argued that the set of secondary effects that affect the galaxy distribution,…

宇宙学与河外天体物理 · 物理学 2018-02-15 Christiane S. Lorenz , David Alonso , Pedro G. Ferreira

The feasibility of a measurement of the electric and magnetic nucleon form factors at $B$-meson factories through the radiative return is studied. Angular distributions allow a separation of the contributions from the two form factors. The…

高能物理 - 唯象学 · 物理学 2010-02-03 Henryk Czyz , Johann H. Kuhn , Elzbieta Nowak , German Rodrigo

In the heavy-quark and large-energy limits, symmetry relations reduce the number of independent form factors governing heavy-to-light $B$-meson decays. Exploiting these relations, the form factors can be parametrized while systematically…

高能物理 - 唯象学 · 物理学 2026-05-11 Saba Ayub , Saba Shafaq , Arslan Sikandar , M. Jamil Aslam

We discuss some nuclear effects, RPA correlations and 2p2h (multinucleon) mechanisms, on charged-current neutrino-nucleus reactions that do not produce a pion in the final state. We study a wide range of neutrino energies, from few hundreds…

高能物理 - 唯象学 · 物理学 2013-10-29 J Nieves , R Gran , F Sanchez , M J Vicente Vacas

We present a consistent calculation of the structure functions within a light-front constituent quark model of the nucleon. Relativistic effects and the relevance of the covariance constraints are analyzed for both polarized and unpolarized…

高能物理 - 唯象学 · 物理学 2009-10-31 P. Faccioli , M. Traini , V. Vento

We study the effects realistic fracture criteria have on crack morphology obtained in numerical simulations with a stochastic discrete element method. Results are obtained with two criteria which are consistent with the theory of elasticity…

软凝聚态物质 · 物理学 2018-08-21 Bjørn Skjetne , Alex Hansen

While the $\Lambda$CDM model succeeds on large scales, its validity on smaller scales remains uncertain. Recent works suggest that non-halo dark matter structures, such as filaments and walls, could significantly influence gravitational…

宇宙学与河外天体物理 · 物理学 2025-05-21 Baptiste Jego , Giulia Despali , Tamara Richardson , Jens Stücker

From a geometrical viewpoint, according to the theory of relativity, space and time constitute a four-dimensional continuum with pseudo-Euclidean structure. This has recently begun to be a practically important statement in accelerator…

经典物理 · 物理学 2017-09-28 Gianluca Geloni , Vitali Kocharyan , Evgeni Saldin

We simulate the fragmentation processes in the \CaCa collisions at the bombarding energy 1.05 GeV/u using the Lorentz covariant RQMD and the non-covariant QMD approaches, incorporated with the statistical decay model. By comparing the…

核理论 · 物理学 2019-08-17 Tomoyuki Maruyama , Toshiki Maruyama , Koji Niita

The strikingly different high energy behaviours of real photoabsorption cross-sections with Q^2 = 0 and the low x proton structure function at large Q^2 are studied from a laboratory frame viewpoint, in which the x and Q^2 dependence…

高能物理 - 唯象学 · 物理学 2009-10-30 G. Kerley , G. Shaw