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Ish: The Cosmological Baryon Density from the Deuterium‐to‐Hydrogen Ratio in QSO Absorption Systems: D/H toward Q1243+3047

1. Constraining Big Bang nucleosynthesis in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi>T</mml:mi> <mml:mo>,</mml:mo> <mml:mi>B</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>T</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="script">G</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="script">G</mml:mi> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> </mml:math> gravity

   Abdul Malik Sultan, Manahil Ali, Shamaila Rani +3

   MaqolaCosmology and Gravitation TheoriesNuclear Physics B20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.001103

2. The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745

   Jean-Paul Breuer, N. Werner, Tomáš Plšek +12

   MaqolaGamma-ray bursts and supernovaeAstronomy and Astrophysics20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.008918