2016
DOI: 10.2140/pjm.2016.285.427
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Bundles of spectra and algebraic K-theory

Abstract: Abstract. A parametrized spectrum E is a family of spectra Ex continuously parametrized by the points x ∈ X of a topological space. We take the point of view that a parametrized spectrum is a bundle-theoretic geometric object. When R is a ring spectrum, we consider parametrized R-module spectra and show that they give cocycles for the cohomology theory determined by the algebraic K-theory K(R) of R in a manner analogous to the description of topological K-theory K 0 (X) as the Grothendieck group of vector bund… Show more

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Cited by 6 publications
(15 citation statements)
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“…This makes it difficult to use the standard machinery to study algebras and modules in this category. These problems have received significant attention in the setting of parametrized stable homotopy theory [62,52,53].…”
Section: ∞-Operadsmentioning
confidence: 99%
“…This makes it difficult to use the standard machinery to study algebras and modules in this category. These problems have received significant attention in the setting of parametrized stable homotopy theory [62,52,53].…”
Section: ∞-Operadsmentioning
confidence: 99%
“…(See for example [27]). To understand the gauge symmetry on the manifold string topology spectrum S • P k (S 4 ) we therefore want to describe the representation…”
Section: Gauge Symmetrymentioning
confidence: 99%
“…Finally, notice that given any compact ring spectrum R, the group of units GL 1 (R) acts on its Spanier-Whitehead dual R ∨ by the dual action of GL 1 (R) on R. Given the Spanier-Whitehead duality between the manifold string topology spectrum S • P k (S 4 ) ≃ (P Ad k ) −T S 4 and the Lie group string topology spectrum S P k • (S 4 ) ≃ (P Ad k ) −Tvert then (27) describes the action of the based gauge group G b (P k ) on the Lie group string topology spectrum as well.…”
Section: Gauge Symmetrymentioning
confidence: 99%
“…With a rate of more than 10 000 spectra per night the pipeline needs to not only provide a robust analysis, but must also be quick and have a reliable performance. Our team has extensive experience in the analysis of stellar spectra in past and ongoing spectroscopic surveys (e.g., Gaia-ESO, RAVE and GALAH) as well as in-depth knowledge about the analysis of stellar spectra including 3D stellar model atmospheres and non-LTE analysis of spectra (Bergemann et al 2012, Lind et al 2012). Currently we are benchmarking various methods (including both physical modelling of stellar spectra as well as data-driven approaches) and working on how to best implement the results from 3D modelling of stellar atmospheres and our better understanding of deviations from LTE in our analysis.…”
Section: Analysis Of Stellar Spectramentioning
confidence: 99%