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Иш: High pressure effects revisited for the cuprate superconductor family with highest critical temperature

1. On the uniaxial strain (pressure) derivatives of the critical temperature of superconductivity of La<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si170.svg" display="inline" id="d1e2055"><mml:msub><mml:mrow/><mml:mrow><mml:mn>2</mml:mn><mml:mo>−</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:msub></mml:math>Sr<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si171.svg" display="inline" id="d1e2067"><mml:msub><mml:mrow/><mml:mrow><mml:mi>x</mml:mi></mml:mrow></mml:msub></mml:math>CuO4

   A.S. Jalekeshov, Bakhrom Yavidov

   МақолаPhysics of Superconductivity and MagnetismPhysica C Superconductivity20223 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.338092

2. A model for calculating the uniaxial pressure derivatives of the critical temperature in Hg-12 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.svg"> <mml:mrow> <mml:mrow> <mml:mo stretchy="true">(</mml:mo> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo linebreak="badbreak">−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> <mml:mo stretchy="true">)</mml:mo> </mml:mrow> <mml:mi>n</mml:mi> </mml:mrow> </mml:math> superconductors: A Casimir energy scenario

   Abdullo Ahadov, D. R. Dzhuraev

   МақолаPhysics of Superconductivity and MagnetismSolid State Communications20251 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001410