A mutual information based R-vine copula strategy to estimate VaR in high frequency stock market data.
Journal
PloS one
ISSN: 1932-6203
Titre abrégé: PLoS One
Pays: United States
ID NLM: 101285081
Informations de publication
Date de publication:
2021
2021
Historique:
received:
25
07
2020
accepted:
03
06
2021
entrez:
17
6
2021
pubmed:
18
6
2021
medline:
17
11
2021
Statut:
epublish
Résumé
In this paper, we explore mutual information based stock networks to build regular vine copula structure on high frequency log returns of stocks and use it for the estimation of Value at Risk (VaR) of a portfolio of stocks. Our model is a data driven model that learns from a high frequency time series data of log returns of top 50 stocks listed on the National Stock Exchange (NSE) in India for the year 2014. The Ljung-Box test revealed the presence of Autocorrelation as well as Heteroscedasticity in the underlying time series data. Analysing the goodness of fit of a number of variants of the GARCH model on each working day of the year 2014, that is, 229 days in all, it was observed that ARMA(1,1)-EGARCH(1,1) demonstrated the best fit. The joint probability distribution of the portfolio is computed by constructed an R-Vine copula structure on the data with the mutual information guided minimum spanning tree as the key building block. The joint PDF is then fed into the Monte-Carlo simulation procedure to compute the VaR. If we replace the mutual information by the Kendall's Tau in the construction of the R-Vine copula structure, the resulting VaR estimations were found to be inferior suggesting the presence of non-linear relationships among stock returns.
Identifiants
pubmed: 34138970
doi: 10.1371/journal.pone.0253307
pii: PONE-D-20-23135
pmc: PMC8211166
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM
Pagination
e0253307Déclaration de conflit d'intérêts
NO authors have competing interests.
Références
PLoS One. 2014 May 07;9(5):e96732
pubmed: 24806471
Phys Rev E Stat Nonlin Soft Matter Phys. 2014 May;89(5):052801
pubmed: 25353838
PLoS One. 2018 Apr 18;13(4):e0195941
pubmed: 29668715
PLoS One. 2019 Aug 29;14(8):e0221910
pubmed: 31465507