Combined experimental and theoretical investigation of the premartensitic transition in NiMnGa
arXiv:0803.2724 · doi:10.1103/PhysRevLett.100.165703
Abstract
Ultraviolet-photoemission (UPS) measurements and supporting specific-heat, thermal-expansion, resistivity and magnetic-moment measurements are reported for the magnetic shape-memory alloy NiMnGa over the temperature range . All measurements detect clear signatures of the premartensitic transition () and the martensitic transition (). Temperature-dependent UPS shows a dramatic depletion of states (pseudogap) at located 0.3eV below the Fermi energy. First-principles electronic structure calculations show that the peak observed at 0.3eV in the UPS spectra for is due to the Ni-d minority-spin electrons. Below this peak disappears, resulting in an enhanced density of states at energies around 0.8eV. This enhancement reflects Ni-d and Mn-d electronic contributions to the majority-spin density of states and is accompanied by significant reconstruction of the Fermi surface.
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