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4 real negative results, null findings, and replication failures in Physics and Astronomy · Failed Experiment Report. Search the index →

WASTE indexes published research — it does not host or republish full papers. Each entry is a metadata record compiled from open scholarly databases; the abstract is shown in full only where the paper is openly licensed, otherwise a short excerpt under fair use. Classifications are automated and approximate.

Failed Experiment ReportOpen accessPhysics and Astronomy

Absence of local moments in the kagome metal KV 3 Sb 5 as determined by muon spin spectroscopy

Eric M Kenney, Brenden R Ortiz, Chennan Wang et al. · 2021 · Journal of Physics Condensed Matter

Abstract We have carried out muon spin relaxation and rotation measurements on the newly discovered kagome metal KV 3 Sb 5 , and find a local field dominated by weak magnetic disorder which we associate with the nuclear moments present,…

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Failed Experiment ReportPhysics and Astronomy

A versatile phenomenological model for the S-shaped temperature dependence of photoluminescence energy for an accurate determination of the exciton localization energy in bulk and quantum well structures

V. K. Dixit, S. Porwal, S. D. Singh et al. · 2014 · Journal of Physics D Applied Physics

Temperature dependence of the photoluminescence (PL) peak energy of bulk and quantum well (QW) structures is studied by using a new phenomenological model for including the effect of localized states. In general an anomalous S-shaped…

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Failed Experiment ReportOpen accessPhysics and Astronomy

Neutrino heating in 1D, 2D, and 3D core-collapse supernovae: characterizing the explosion of high-compactness stars

Luca Boccioli, David Vartanyan, Evan O’Connor et al. · 2025 · Monthly Notices of the Royal Astronomical Society

ABSTRACT Massive stars can end their lives with a successful supernova explosion (leaving behind a neutron star or, more rarely, a black hole), or a failed explosion that leaves behind a black hole. The density structure of the pre-collapse progenitor star already encodes much of the information regarding the outcome and properties of the explosion. However, the complexity of the collapse and subsequent shock expansion phases prevents drawing a straightforward connection between the pre-collapse and post-explosion properties. In order to derive such a connection several explodability studies h

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