On the E^1-term of the gravity spectral sequence
| dc.creator | Tamaki, Dai | |
| dc.date | 2009-03-26 | |
| dc.date.accessioned | 2026-07-07T12:57:27Z | |
| dc.date.available | 2026-07-07T12:57:27Z | |
| dc.description | The author constructed a spectral sequence strongly converging to h_*(Omega^n Sigma^n X) for any homology theory in [Topology 33 (1994) 631-662]. In this note, we prove that the E^1-term of the spectral sequence is isomorphic to the cobar construction, and hence the spectral sequence is isomorphic to the classical cobar-type Eilenberg-Moore spectral sequence based on the geometric cobar construction from the E^1-term. Similar arguments can be also applied to its variants constructed in [Contemp Math 293 (2002) 299-329]. | |
| dc.description | This is the version published by Geometry & Topology Monographs on 18 April 2007 | |
| dc.identifier | https://arxiv.org/abs/0903.4704 | |
| dc.identifier | http://arxiv.org/abs/0903.4704 | |
| dc.identifier | Geom. Topol. Monogr. 10 (2007) 347-382 | |
| dc.identifier | doi:10.2140/gtm.2007.10.347 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/224936 | |
| dc.subject | Algebraic Topology | |
| dc.subject | 55T20, 55P48 | |
| dc.title | On the E^1-term of the gravity spectral sequence | |
| dc.type | text |