dc.contributor.author | Allez, Romain | |
dc.contributor.author | Bouchaud, Jean-Philippe | |
dc.date.accessioned | 2013-01-28T14:46:29Z | |
dc.date.available | 2013-01-28T14:46:29Z | |
dc.date.issued | 2011 | |
dc.identifier.uri | https://basepub.dauphine.fr/handle/123456789/10898 | |
dc.language.iso | en | en |
dc.subject | Computational physics | en |
dc.subject | Statistical physics and nonlinear systems | en |
dc.subject | Statistical Finance | en |
dc.subject.ddc | 519 | |
dc.subject.classificationjel | G1 | |
dc.title | Individual and collective stock dynamics: intra-day seasonalities | en |
dc.type | Article accepté pour publication ou publié | |
dc.description.abstracten | We establish several new stylized facts concerning the intra-day seasonalities of stock dynamics. Beyond the well-known U-shaped pattern of the volatility, we find that the average correlation between stocks increases throughout the day, leading to a smaller relative dispersion between stocks. Somewhat paradoxically, the kurtosis (a measure of volatility surprises) reaches a minimum at the open of the market, when the volatility is at its peak. We confirm that the dispersion kurtosis is a markedly decreasing function of the index return. This means that during large market swings, the idiosyncratic component of the stock dynamics becomes sub-dominant. In a nutshell, the early hours of trading are dominated by idiosyncratic or sector-specific effects with little surprises, whereas the influence of the market factor increases throughout the day, and surprises become more frequent. | en |
dc.relation.isversionofjnlname | New Journal of Physics | |
dc.relation.isversionofjnlvol | 13 | en |
dc.relation.isversionofjnldate | 2011 | |
dc.relation.isversionofjnlpages | n°025010 | en |
dc.relation.isversionofdoi | http://dx.doi.org/10.1088/1367-2630/13/2/025010 | en |
dc.identifier.urlsite | http://arxiv.org/abs/1009.4785 | en |
dc.relation.isversionofjnlpublisher | IOP Science | en |
dc.subject.ddclabel | Probabilités et mathématiques appliquées | |
dc.relation.forthcoming | non | en |
dc.relation.forthcomingprint | non | en |