Time Diversification#

Notation#

notation

description

\(r_t\)

return rate, (\(t-1\) to \(t\))

\(r_{t,t+h}\)

\(\left(\prod_{\tau=1}^h R_{t+\tau}\right)-1\)

\(r^{\log}_t\)

\(\log\left(1+r_t\right)\)

\(r^{\log}_{t,t+h}\)

\(\log\left(1+r_{t,t+h}\right)\)

Cumulative Return Risk and Autocorrelation#

Log cumulative returns are simply a portfolio of single-period returns.

  • Define \(\mu\) and \(\sigma^2\) as $\(\mathbb{E}\left[r^{\log}_{t,t+1}\right] = \mu, \quad \text{Var}\left[r^{\log}_{t,t+1}\right] = \sigma^2\)$

  • For the \(h\)-period log return, $\(\mathbb{E}\left[r^{\log}_{t,t+h}\right] = h\mu\)\( \)\(\text{Var}\left[r^{\log}_{t,t+h}\right] = \sum_{j=1}^h\sum_{i=1}^h \text{Cov}\left[r^{\log}_{t+i},r^{\log}_{t+j}\right]\)$

Like the case of diversifying one-period returns across \(k\) assets, the covariances determine the overall risk but do not affect the mean return.

Autocorrelation Models#

As seen in the previous section,

  • The variance of cumulative returns, \(r^{\log}_{t,t+h}\), depends critically on the auto-covariance of the return series, denoted as $\(\text{Cov}\left[r^{\log}_{t},r^{\log}_{t+i}\right], \quad \text{or} \quad \sigma_{t,t+i}\)$

  • Specifying a form for the autocorrelations, \(\text{Corr}\left[r^{\log}_{t},r^{\log}_{t+i}\right]\), is equivalent.

  • A model of autocorrelations uniquely specifies a linear time series model.

AR(1) Models#

Autoregressive (AR) models are among the most popular in time-series statistics.

Consider the AR(1) model, $\(\text{Cov}\left[r^{\log}_{t},r^{\log}_{t+i}\right] = \rho^i \sigma^2\)\( \)\(\text{Corr}\left[r^{\log}_{t},r^{\log}_{t+i}\right] = \rho^i\)$

With AR models, covariances are easy to scale over time.

Diversification and Cumulative Returns#

Mean returns scale linearly in horizon \(h\), $\(\mathbb{E}\left[r^{\log}_{t,t+h}\right] = h\mu\)$

But scaling of variance depends on correlation:

  • \(\rho=1\): Std.Dev. is linear in cumulation: \(\text{Std}\left[r^{\log}_{t,t+h}\right] = h\sigma\)

  • \(\rho=0\): Variance is linear in cumulation: \(\text{Var}\left[r^{\log}_{t,t+h}\right] = h\sigma^2\)

  • \(\rho=-1\): The return is riskless: \(\text{Var}\left[r^{\log}_{t,t+h}\right] = 0\)

Example: Riskless Bond#

At time \(t=0\), consider a bond with riskless payout at \(t=10\). The yield of the bond at \(t=0\) is 5%.

  • The 10-year cumulative return, \(r^{\log}_{0,10}\) is riskless, and equals \(5\% \times 10\).

  • At any intermediate time, (\(t\), such that \(0< t < 10\),) the bond price is uncertain.

  • Thus, the intermediate returns, \(r^{\log}_{0,t}\) and \(r^{\log}_{t,10}\) are uncertain.

  • However, \(r^{\log}_{0,10} = r^{\log}_{0,t} + r^{\log}_{t,10}\).

  • So if \(r^{\log}_{0,t}\) is unexpectedly high, then \(r^{\log}_{t,10}\) must be relatively low, such that the riskless return \(r^{\log}_{0,10}\) ends up at \(5\%\times 10\).

Example: Bond Mean Reversion#

A ten-year risk-free bond has a 10-year return with perfect mean reversion. (Source: Cochrane, 2011)

Bond mean reversion demo

Negative Serial Correlation in Bonds#

Thus, riskless bonds should have negatively autocorrelated returns: $\(\text{Corr}\left(r^{\log}_t,r^{\log}_{t+1}\right)<0\)$

And if the bond matures at \(T\), then for any \(0<h<T-t\), $\(\text{Corr}\left(r^{\log}_{t,t+h},r^{\log}_{t+h,T}\right) = -1\)$

Default-free bonds are safer in the long-run, with \(\text{Var}\left[r^{\log}_{t,T}\right]=0\).

Cumulative Sharpe Ratios in AR(1) Model#

Consider again the cumulative return, \(r^{\log}_{t,t+h}\).

  • For \(\rho=1\): $\(\text{SR}\left(r^{\log}_{t,t+h}\right) = \text{SR}\left(r^{\log}_t\right)\)$

  • For \(|\rho|<1\): $\(\text{SR}\left(r^{\log}_{t,t+h}\right) > \text{SR}\left(r^{\log}_t\right)\)$

  • For \(\rho=0\): $\(\text{SR}\left(r^{\log}_{t,t+h}\right) = \sqrt{h}~ \text{SR}\left(r^{\log}_t\right)\)$

Mean Annualized Returns#

The annualized mean (log) return on the \(h\)-period investment, \(r^{\log}_{t,t+h}\) is

\[\frac{r^{\log}_{t,t+h}}{h} = \frac{\sum_{i=1}^h r^{\log}_{t+i}}{h}\]

This is just the usual sample estimate of the mean of one-period returns, \(\bar{r}\), based on a sample-size of \(h\)!

For any \(\rho\)

For \(\rho=0\)

\(\mathbb{E}\left[\bar{r}\right] = \mu\)

\(\text{Var}\left[\bar{r}\right] = \frac{\sigma^2}{h}\)

  • So as the investment horizons gets large, the mean annualized return, \(\bar{r}\), converges to the true annual mean return, \(\mu\).

  • Even if \(\rho\ne 0\) we can still conclude that \(\bar{r}\to \mu\). (Law of large numbers still holds.)

Time Diversification#

Time-diversification refers to this idea that mean annualized return becomes riskless for large investment horizons.

  • True, as horizon increases the variance of the annualized return goes to zero.

  • However, the variance of the cumulative return, \(r^{\log}_{t,t+h}\) is still growing.

So-called time diversification depends on the risk one is measuring.

Evidence: Are Equity Returns Serially Correlated?#

Table: Auto-regression estimates for market returns, risk-free rate, and excess market returns. Regression estimates of \(y_{t+1}= a +\rho y_t +\epsilon_{t+1}\)

\(y=\ldots\)

Monthly

Annual

\(r_{mkt}\)

\(r_f\)

\(rx_{mkt}\)

\(r_{mkt}\)

\(r_f\)

\(rx_{mkt}\)

\(\hat{\rho}\)

0.11

0.89

0.12

0.01

0.92

0.02

\(t(\hat{\rho})\)

2.02

30.38

2.05

0.09

13.31

0.15

\(R^2\)

0.01

0.80

0.01

0.00

0.83

0.00

Source: CRSP value-weighted equity markets, 1927-2010. CRSP 3-month U.S. treasury bill. GMM standard errors.

Serial Correlation of Equities#

  • The table shows that empirically the serial correlation of excess equity returns is small.

  • Not surprisingly, the serial correlation of the risk-free rate is very high.

  • The serial correlation is much smaller for annual returns.

Does estimating the autocorrelation of longer-horizon returns tell a different story?

Evidence: Cumulative Equity Returns#

Table: Std.dev., Sharpe-ratios, and serial correlation, of excess cumulative returns.

h (years)

1

3

5

7

10

\(\sigma/\sqrt{h}\)

0.21

0.24

0.28

0.26

0.32

\(SR/\sqrt{h}\)

0.36

0.36

0.32

0.34

0.30

\(\hat{\rho}\)

0.01

-0.29

-0.30

0.40

0.06

  • \(h\)-year excess return of the CRSP U.S. equity index over the 90-day t-bill.

  • \(\hat{\rho}\) is the sample estimate of serial correlation of long-horizon excess returns.

Long-run Uncertainty#

  • The results in the table above show that normalized by \(\sqrt{h}\), the Sharpe ratios remain almost constant across return horizon, or slightly decrease.

  • This would be consistent with market equity excess returns having small serial correlation.

  • Unfortunately, the basic estimates in the previous table are not statistically conclusive.

  • Not surprising, since there are not a lot of long-horizon data points available.