The Role of Inventories and Speculative Trading in the Global Market for Crude Oil
University of Michigan at Ann Arbor - Department of Economics; Centre for Economic Policy Research (CEPR)
University of Michigan at Ann Arbor
CEPR Discussion Paper No. DP7753
We develop a structural model of the global market for crude oil that for the first time explicitly allows for shocks to the speculative demand for oil as well as shocks to the flow demand and flow supply. The forward-looking element of the real price of oil is identified with the help of data on oil inventories. The model estimates rule out explanations of the 2003-08 oil price surge based on unexpectedly diminishing oil supplies and based on speculative trading. Instead, we find that this surge was caused by fluctuations in the flow demand for oil driven by the global business cycle. There is evidence, however, that speculative demand shifts played an important role during earlier oil price shock episodes including 1979, 1986, and 1990. Recently, it has been suggested that it is possible for speculative trading to occur even without any change in oil inventories, if the short-run price elasticity of oil demand is zero. Our structural model allows us to obtain an estimate of this elasticity based on shifts of the supply curve along the demand curve. We show that, even after accounting for the role of inventories in smoothing oil consumption, our estimate of the price elasticity of oil demand is not close to zero and much higher than traditional estimates from dynamic models that do not account for price endogeneity. This eliminates speculation as an explanation of the 2003-08 oil price surge.
Number of Pages in PDF File: 45
Keywords: demand, fundamentals, gasoline demand elasticity, identification, inventories, oil demand elasticity, Oil market, peak oil, speculation, structural model, supply
JEL Classification: D84working papers series
Date posted: March 29, 2010
© 2014 Social Science Electronic Publishing, Inc. All Rights Reserved.
This page was processed by apollo3 in 1.125 seconds