Cited by 27High Entropy Alloys StudiesPhysics of Superconductivity and MagnetismSuperconducting Materials and Applications

Superconductivity with a high upper critical field in an equiatomic high-entropy alloy Sc–V–Ti–Hf–Nb

Jangid, S., Meena, P. K., Kushwaha, R. K., Srivastava, S., Manna, P., Mishra, P., Sharma, S., Singh, R. P.·2024·Applied Physics Letters

Abstract

High-entropy alloy (HEA) superconductors have attracted significant attention due to their exceptional low-temperature mechanical and superconducting properties. We report the synthesis and thorough characterization of an equiatomic HEA superconductor with the composition Sc0.20V0.20Ti0.20Hf0.20Nb0.20, crystallizing in a body-centered cubic crystal structure (Im3m¯). Our investigation, using magnetization, transport, and heat capacity measurements, reveals the presence of weakly coupled, fully gapped superconductivity with a transition temperature of 4.17(3) K and the upper critical field exceeding the Pauli paramagnetic limit. The metallic nature, combined with a high upper critical field, positions it as a promising candidate for applications in superconducting devices.

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Crossref · 10.1063/5.0200805

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  • The μ0Hc2(0) exceeding the Pauli paramagnetic limit was also found in BCC-type ScVTiHfNb, HCP-type Ru0.35Os0.35Mo0.12W0.1Zr0.1, A15-type (Nb0.5V0.5)3-xMoxAl0.5Ga0.5, and α-Mn-type Ru0.35Os0.35Mo0.1W0.1Zr0.1 HEA superconductors.

    “The μ 0Hc2(0) exceeding the Pauli paramagnetic limit was also found in BCC-type ScVTiHfNb 21 , HCP-type Ru0.35Os0.35Mo0.12W0.1Zr0.1 89 , A15-type (Nb0.5V0.5)3x Mo x Al0.5Ga0.5 57 , and α -Mn-type Ru0.35Os0.35Mo0.1W0.1Zr0.1 HEA superconductors 89 .”

    From Recent advances in high-entropy superconductors (2024) · cites this paper as [21]

  • The Maki parameter αM is 1.05 for the ScVTiHfNb HEA superconductor.

    “The Maki parameter α M is 1.05 for the ScVTiHfNb HEA superconductor 21 .”

    From Recent advances in high-entropy superconductors (2024) · cites this paper as [21]

  • Depending on the αM value, pair breaking is due primarily to the Pauli paramagnetic effect, with a small contribution from the orbital limiting effect.

    “Depending on the α M value, pair breaking is due primarily to the Pauli paramagnetic effect, with a small contribution from the orbital limiting effect.”

    From Recent advances in high-entropy superconductors (2024) · cites this paper as [21]

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Authors
Jangid, S., Meena, P. K., Kushwaha, R. K., Srivastava, S., Manna, P., Mishra, P., Sharma, S., & Singh, R. P.
Affiliations
Indian Institute of Science Education and Research, Bhopal (IN)
Corresponding author
Singh, R. P.
Venue
Applied Physics Letters
Published
2024-05-06
Volume
124
Issue
19
ISSN
  • 0003-6951 (ISSN-L)
  • 1077-3118
OpenAlex
W4396760947
Cited by
27
References
10
Citations by year
2026: 7 · 2025: 17 · 2024: 3
FWCI
3.60
Type
journal article
Language
en
Open access
closed
Locations
Applied Physics Letters (publishedVersion)
Funders
Science and Engineering Research Board (CRG/2019/001028)
Topics
  • Physical Sciences › Engineering › Mechanical Engineering › High Entropy Alloys Studies
  • Physical Sciences › Physics and Astronomy › Condensed Matter Physics › Physics of Superconductivity and Magnetism
  • Physical Sciences › Engineering › Biomedical Engineering › Superconducting Materials and Applications
Keywords
high-entropy alloys, superconductivity, upper critical field, equiatomic alloys, body-centered cubic lattice, Pauli paramagnetic limit, weak-coupling superconductivity, superconducting gap, low-temperature superconductors, heat capacity, magnetization, electrical transport

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