1,093 research outputs found

    Jason Casanova, euphonium

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    KSU School of Music presents Jason Casanova, euphonium and Eric Jenkins, pianohttps://digitalcommons.kennesaw.edu/musicprograms/2233/thumbnail.jp

    (η5-Cyclo­penta­dien­yl)[η6-diethyl eth­yl(phen­yl)malonate]iron(II) hexa­fluorido­phosphate

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    At 223 (2) K, the complexed rings in the iron(II) complex cation of the title salt, [Fe(C5H5)(C15H20O4)]PF6, are almost parallel [dihedral angle between planes = 4.10 (14)°]. Among the C atoms of the complexed arene ring, the quaternary C atom is located at the longest distance from the Fe atom. The F atoms of the PF6 − anion were found to be equally disordered over two sites

    (η5-Cyclo­penta­dien­yl)(η6-1,2-dipyrrolidin-1-ylbenzene)iron(II) hexa­fluoridophosphate

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    Both complexed rings in the iron(II) complex cation of the title salt, [Fe(C5H5)(C14H20N2)]PF6, are almost parallel [dihedral angle between planes = 5.34 (13)°]. Among the C atoms of the complexed arene ring, the quaternary C atoms are located at the longest, albeit unequal, distances from the Fe atom [2.252 (2) and 2.168 (2) Å]

    Dark matter effective field theory and an application to vector dark matter

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    The Standard Model Effective Field Theory (SMEFT) and the Low Energy Effective Field Theory (LEFT) can be extended by adding additional spin 0, 1/2 and 1 dark matter particles which are singlets under the Standard Model (SM) gauge group. We classify all gauge invariant interactions in the Lagrangian up to terms of dimension six, and present the tree-level matching conditions between the two theories at the electroweak scale. The most widely studied dark matter models, such as those based on the Higgs portal or on kinetic mixing between the photon and a dark photon, are based on dimension-four interactions with the SM sector. We consider a model with dark vector particles with a ℤ2 symmetry, so that the lightest dark matter particle is stable. The leading interaction with the SM is through dimension-six operators involving two dark vector field-strength tensors and the electromagnetic field-strength tensor. This model is a viable dark matter model in the freeze-in scenario for a wide range of parameters
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