Mechanisms of Shock Strength Exhibited by a Nickel‐Rich Nickel‐Titanium‐Hafnium Alloy

Author:

Knapp Tyler1,Amin-Ahmadi Behnam2,Turnage Scott3,Mills Sean H.4,Thadhani Naresh N.1,Noebe Ronald D.5,Williams Cyril L.3,Stebner Aaron P.16ORCID

Affiliation:

1. Materials Science and Engineering Georgia Institute of Technology Atlanta GA 30313 USA

2. Confluent Medical Technologies Fremont CA 94539 USA

3. Applied Physics Branch U.S. Army Research Laboratory Aberdeen MD 21005 USA

4. Materials Science and Engineering University of California Berkeley CA 94720 USA

5. NASA Glenn Research Center Materials and Structures Division Cleveland OH 44135 USA

6. G. W. Woodruff School of Mechanical Engineering Georgia Institute of Technology Atlanta GA 30313 USA

Abstract

Nickel‐rich NiTiHf alloys that are heat treated to strengthen the microstructures with a dense distribution of Ni4Ti3 nanoprecipitates exhibit very high strengths and good quasi‐static indentation resistance and rolling contact fatigue performances. To determine whether these properties are maintained at high rates of loading, in situ and recovery flyer plate impact shock experiments are performed on a Ni54Ti45Hf1 alloy at impact velocities ranging from approximately 150 m s−1 (2.5 GPa) to 700 m s−1 (12.40 GPa). Analysis of shocked samples indicated less cracking is observed to emanate from spall failures resulting from impact velocities greater than 250 m s−1 (4.23 GPa), concurrent with observations of intragranular microbands within the microstructures. Analyses show clear evidence that, like responses to quasi‐static loading, martensitic phase transformation occurs upon shock compression in all cases. However, dissimilarly, for the higher impact velocities it reverses upon stress release, leaving behind microbands that show no evidence for retained martensite and within which the Ni4Ti3 nanoprecipitates dissolved. These results indicate that strain‐rate dependence of these SMAs under shock loading is not only governed by the expected physics of rate‐dependence of the martensitic transformations themselves but may also be enhanced by inelastic deformation mechanisms that result in precipitate dissolution.

Funder

Glenn Research Center

Publisher

Wiley

Subject

Condensed Matter Physics,General Materials Science

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