Abstract

 
 

References (37)



 
 

Citations (6)



 


 



Risk Neutral Probabilities and Option Bounds: A Geometric Approach


James Huang


Lancaster University - Department of Accounting and Finance

February 28, 2005

Lancaster University Management School Working Paper No. 2004/052, EFA 2005 Moscow Meetings Paper

Abstract:     
In this paper we first present a geometric approach to option bounds. We show that if two risk neutral probability density functions intersect for certain number of times, then comparing the fatness of their tails we can tell which of them gives higher option prices. Thus we can derive option bounds by identifying the risk neutral probability density function which intersects all admissible ones for certain number of times. Applying this approach we tighten the first order stochastic dominance option bounds when the maximum value of the risk neutral density is known. The method present in this paper has wide applications in option pricing problems.

Number of Pages in PDF File: 58

Keywords: Option bounds, option pricing, risk neutral density, first order stochastic dominance

JEL Classification: G13

working papers series


Download This Paper

Date posted: March 6, 2005  

Suggested Citation

Huang, James, Risk Neutral Probabilities and Option Bounds: A Geometric Approach (February 28, 2005). Lancaster University Management School Working Paper No. 2004/052, EFA 2005 Moscow Meetings Paper. Available at SSRN: http://ssrn.com/abstract=621663 or http://dx.doi.org/10.2139/ssrn.621663

Contact Information

James Xiaoping Huang (Contact Author)
Lancaster University - Department of Accounting and Finance ( email )
The Management School
Lancaster LA1 4YX
United Kingdom
01 5245 93633 (Phone)
01 5248 47321 (Fax)
Feedback to SSRN (Beta)


Paper statistics
Abstract Views: 1,260
Downloads: 202
Download Rank: 40,899
References:  37
Citations:  6

© 2013 Social Science Electronic Publishing, Inc. All Rights Reserved.  FAQ   Terms of Use   Privacy Policy   Copyright
This page was processed by apollo1 in 0.454 seconds