Optical properties and electronic structures of B2 and B19′ phases of equiatomic Ni-Ti alloys

Thumbnail Image
Date
1999
Authors
Rhee, Joo
Harmon, Bruce
Lynch, David
Major Professor
Advisor
Committee Member
Journal Title
Journal ISSN
Volume Title
Publisher
Authors
Person
Research Projects
Organizational Units
Organizational Unit
Physics and Astronomy
Physics and astronomy are basic natural sciences which attempt to describe and provide an understanding of both our world and our universe. Physics serves as the underpinning of many different disciplines including the other natural sciences and technological areas.
Journal Issue
Is Version Of
Versions
Series
Department
Physics and Astronomy
Abstract

The dielectric functions of equiatomic Ni-Ti alloys were measured by spectroscopic ellipsometry in the energy range of 1.5–5.4 eV at ∼423 and at ∼25 K. The peak at ∼2.26 eV in the B19′ (monoclinic structure) optical conductivity spectrum has a slightly larger magnitude than in the B2 (cubic CsCl structure) phase, while the shoulder at ∼3.5 eVbecomes weaker and almost indiscernible upon martensitic transformation. A new structure develops at ∼2.85 eV in the B19′ phase; however, it is also very weak. The band structures and the optical conductivity were calculated in both phases using the linearized-augmented-plane-wave method within the local-density approximation. k points near the Γ−X−M plane in the B2 phase and the corresponding k-points in B19′ phase contribute significantly to all three structures. The difference between the two spectra is due to the transitions between the folded-back bands from the B2phase because of the larger unit cell of the B19′ phase and the change in the electronic energy spectrum near the Fermi level. The overall optical properties of Ni-Ti alloys in the measured energy range are rather insensitive to the martensitic transformation because the states far from the Fermi level are mainly involved in the interband transitions.

Comments

This article is from Physical Review B 59 (1999): 1878, doi:10.1103/PhysRevB.59.1878. Posted with permission.

Description
Keywords
Citation
DOI
Copyright
Fri Jan 01 00:00:00 UTC 1999
Collections