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1. Superhalogens Among 3 d -Metal Compounds: M F ₄ , M F ₆ , M F ₁₂ , and M F ₁₈ ( M = Sc–Zn)

   https://doi.org/10.1021/acs.jpca.1c02884  

   Gutsev, Gennady L.; Tibbetts, Katharine M.; Gutsev, Lavrenty G.; Ramachandran, Bala R. (May 2021, The Journal of Physical Chemistry A)
2. VOA[ M ₄ ]

   https://doi.org/10.1063/1.5100059  

   Feigin, Boris; Gukov, Sergei (January 2020, Journal of Mathematical Physics)
3. Kinetics of the Topochemical Transformation of (PbSe) _m (TiSe ₂ ) _n (SnSe ₂ ) _m (TiSe ₂ ) _n to (Pb _0.5 Sn _0.5 Se) _m (TiSe ₂ ) _n

   https://doi.org/10.1021/jacs.8b10681  

   Sutherland, Duncan R.; Merrill, Devin R.; Ditto, Jeffrey; Moore, Daniel B.; Medlin, Douglas; Johnson, David C. (January 2019, Journal of the American Chemical Society)
4. Inferring M _BH – M _bulge Evolution from the Gravitational-wave Background

   https://doi.org/10.3847/1538-4357/ae2480  

   Matt, Cayenne; Gültekin, Kayhan; Kelley, Luke Zoltan; Blecha, Laura; Simon, Joseph; Agazie, Gabriella; Anumarlapudi, Akash; Archibald, Anne M; Arzoumanian, Zaven; Baier, Jeremy G; et al (January 2026, The Astrophysical Journal)

   Abstract We test the impact of an evolving supermassive black hole mass scaling relation (M_BH–M_bulge) on the predictions for the gravitational-wave background (GWB). The observed GWB amplitude is 2–3 times higher than predicted by astrophysically informed models, which suggests the need to revise the assumptions in those models. We compare a semi-analytic model’s ability to reproduce the observed GWB spectrum with a static versus evolving-amplitudeM_BH–M_bulgerelation. We additionally consider the influence of the choice of galaxy stellar mass function (GSMF) on the modeled GWB spectra. Our models are able to reproduce the GWB amplitude with either a large number density of massive galaxies or a positively evolvingM_BH–M_bulgeamplitude (i.e., theM_BH/M_bulgeratio was higher in the past). If we assume that theM_BH–M_bulgeamplitude does not evolve, our models require a GSMF that implies an undetected population of massive galaxies (M_⋆≥ 10¹¹M_⊙atz> 1). When theM_BH–M_bulgeamplitude is allowed to evolve, we can model the GWB spectrum with all fiducial values and anM_BH–M_bulgeamplitude that evolves asα(z) =α₀(1 +z)^1.04±0.5. 

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5. Kinetically Controlled Formation and Decomposition of Metastable [(BiSe) _1+δ ] _m [TiSe ₂ ] _m Compounds

   https://doi.org/10.1021/jacs.7b13398  

   Lygo, Alexander C.; Hamann, Danielle M.; Moore, Daniel B.; Merrill, Devin R.; Ditto, Jeffrey; Esters, Marco; Orlowicz, Jacob; Wood, Suzannah R.; Johnson, David C. (February 2018, Journal of the American Chemical Society)