Published December 31, 2004 | Version v1
Journal article

Magnetic properties of Ni-Rh clusters: Behavior in the Ni-rich region

  • 1. U.A. Fisica, Centro Atomico Constituyentes, Comision Nacional de Energia Atomica, Avda Gral Paz 1499 1560, San Martin, Buenos Aires (Argentina)
  • 2. Escuela de Ciencia y Tecnologia, Universidad de San Martin, Alem 3901, 1563 San Martin (Argentina)

Description

We study the magnetic properties of bimetallic Ni-Rh 55-atom clusters in the Ni-rich region as a function of Rh composition. The minimum energy structures are taken from Molecular Dynamics Simulations by using empirical potentials (in the Second Moment Approximation). We then calculate the electronic and magnetic properties of these structures by using a tight-binding Hamiltonian. The magnetic solutions are found solving a Hubbard-like Hamiltonian within the unrestricted Hartree-Fock Approximation. Bulk parameters and Andersen's exponential law for the dependence of hopping on distance are being used. We obtain that a small number of Rh atoms can modify the average magnetic moment, μ, depending not only on the positions of the Rh atoms (either on the surface-, middle-, or central-shell) but also on their relative positions. The magnetic moment curve corresponding to the minimum energy structures shows a minimum for 2 Rh atoms and there is an enhancement of μ up to 6 Rh atoms, being the μ value of this last cluster even higher than the one corresponding to Ni55 clusters

Additional details

Identifiers

DOI
10.1016/j.physb.2004.09.101;
PII
S0921-4526(04)00967-6;

Publishing Information

Journal Title
Physica. B, Condensed Matter
Journal Volume
354
Journal Issue
1-4
Journal Page Range
p. 303-306
ISSN
0921-4526
CODEN
PHYBE3

Conference

Title
Magnetism, magnetic materials, and their applications
Acronym
Workshop on 'At the frontiers of condensed matter'
Dates
22-26 Jun 2004
Place
Buenos Aires (Argentina)

Optional Information

Copyright
Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.