Log-normal and normal distribution conversion
$c_R,R_f$ are known (constant part of return and risk free rate). Let $R=R_f(e^r-1)=c_R+epsilon_R$, $rsim N(mu_r,sigma_r)$, how to specify the distribution of $epsilon_Rsim Lognormal(?,?)$ by mean and variance of a normal distribution?
probability statistics finance
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$c_R,R_f$ are known (constant part of return and risk free rate). Let $R=R_f(e^r-1)=c_R+epsilon_R$, $rsim N(mu_r,sigma_r)$, how to specify the distribution of $epsilon_Rsim Lognormal(?,?)$ by mean and variance of a normal distribution?
probability statistics finance
add a comment |
$c_R,R_f$ are known (constant part of return and risk free rate). Let $R=R_f(e^r-1)=c_R+epsilon_R$, $rsim N(mu_r,sigma_r)$, how to specify the distribution of $epsilon_Rsim Lognormal(?,?)$ by mean and variance of a normal distribution?
probability statistics finance
$c_R,R_f$ are known (constant part of return and risk free rate). Let $R=R_f(e^r-1)=c_R+epsilon_R$, $rsim N(mu_r,sigma_r)$, how to specify the distribution of $epsilon_Rsim Lognormal(?,?)$ by mean and variance of a normal distribution?
probability statistics finance
probability statistics finance
asked Aug 7 '17 at 4:36
ZHUZHU
406316
406316
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2 Answers
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You specify the distribution of a Lognormal variable with the mean and the variance (or standard deviation) with the parameters of the Normal distribution used to derive the Lognormal distribution.
By definition of the Lognormal variable (https://en.wikipedia.org/wiki/Log-normal_distribution) you would have: $$rsim N(mu_r, sigma_r) Rightarrow e^r =epsilon_r sim LogNormal (mu_r, sigma_r )$$
I never came across an author that specifies $Ysim Lognormal(E[Y],sqrt{Var[Y]})$
add a comment |
Using your notation, we have:
$$R=R_{f}(e^{r}-1)=R_{f},e^{r}-R_{f}$$
where
$$rsim N(mu_{r},sigma_{r})$$
Now, we also know that if $r$ has a normal distribution, then $e^{r}$ is log-normally distributed:
$$e^{r}sim LN(mu_{r},sigma_{r})$$
Furthermore, by scaling $e^{r}$ by $R_{f}$ we arrive at:
$$R_{f},e^{r}sim LN(mu_{r}+text{ln}(R_{f}),sigma_{r})$$
Finally, we subtract the constant $R_{f}$ from the above term:
$$R_{f},e^{r}-R_{f}$$
Now, because the standard log-normal distribution is a 2-parameter distribution with support on $xin(0,infty)$, it needs to be adapted to account for the negative shift of $R_{f}$.
So, we now consider the 3-parameter log-normal distribution, which includes a location parameter, $theta$. Essentially, this adjusts the support of the distribution to be $xin(theta,infty)$. It has probability density function:
$$f_{X}(x;mu,sigma,theta)=frac{1}{(x-theta)sigmasqrt{2pi}}e^{frac{(text{ln}(x-theta)-mu)^{2}}{2sigma^{2}}}$$
where $x>theta,,sigma>0$. The mean and variance of the shifted log-normal distribution are easy enough to calculate. The mean is equal to the mean of the non-shifted log-normal plus the shift:
$$E[X+c]=E[X]+c$$
Similarly, the variance is equal to the variance of the non-shifted log-normal:
$$text{Var}(X+c)=text{Var}(X)$$
So we arrive at:
$$R=R_{f}(e^{r}-1)sim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
with probability density function:
$$f_{R}(r;mu,sigma,theta)=frac{1}{(r+R_{f})sigma_{r}sqrt{2pi}}e^{frac{big(text{ln}(r+R_{f})-mu_{r}-text{ln}(R_{f})big)^{2}}{2sigma_{r}^{2}}}$$
So to answer your question, for the equation:
$$R=c_{R}+epsilon_{R}$$
the value of $c_{R}$ is completely dependent on how you specify the parameters of $epsilon_{R}$. You can have:
$$c_{R}=0,,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
or
$$c_{R}=-R_{f},,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},0)$$
etc.
add a comment |
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2 Answers
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2 Answers
2
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You specify the distribution of a Lognormal variable with the mean and the variance (or standard deviation) with the parameters of the Normal distribution used to derive the Lognormal distribution.
By definition of the Lognormal variable (https://en.wikipedia.org/wiki/Log-normal_distribution) you would have: $$rsim N(mu_r, sigma_r) Rightarrow e^r =epsilon_r sim LogNormal (mu_r, sigma_r )$$
I never came across an author that specifies $Ysim Lognormal(E[Y],sqrt{Var[Y]})$
add a comment |
You specify the distribution of a Lognormal variable with the mean and the variance (or standard deviation) with the parameters of the Normal distribution used to derive the Lognormal distribution.
By definition of the Lognormal variable (https://en.wikipedia.org/wiki/Log-normal_distribution) you would have: $$rsim N(mu_r, sigma_r) Rightarrow e^r =epsilon_r sim LogNormal (mu_r, sigma_r )$$
I never came across an author that specifies $Ysim Lognormal(E[Y],sqrt{Var[Y]})$
add a comment |
You specify the distribution of a Lognormal variable with the mean and the variance (or standard deviation) with the parameters of the Normal distribution used to derive the Lognormal distribution.
By definition of the Lognormal variable (https://en.wikipedia.org/wiki/Log-normal_distribution) you would have: $$rsim N(mu_r, sigma_r) Rightarrow e^r =epsilon_r sim LogNormal (mu_r, sigma_r )$$
I never came across an author that specifies $Ysim Lognormal(E[Y],sqrt{Var[Y]})$
You specify the distribution of a Lognormal variable with the mean and the variance (or standard deviation) with the parameters of the Normal distribution used to derive the Lognormal distribution.
By definition of the Lognormal variable (https://en.wikipedia.org/wiki/Log-normal_distribution) you would have: $$rsim N(mu_r, sigma_r) Rightarrow e^r =epsilon_r sim LogNormal (mu_r, sigma_r )$$
I never came across an author that specifies $Ysim Lognormal(E[Y],sqrt{Var[Y]})$
answered Aug 7 '17 at 6:16
RandowMalkRandowMalk
9510
9510
add a comment |
add a comment |
Using your notation, we have:
$$R=R_{f}(e^{r}-1)=R_{f},e^{r}-R_{f}$$
where
$$rsim N(mu_{r},sigma_{r})$$
Now, we also know that if $r$ has a normal distribution, then $e^{r}$ is log-normally distributed:
$$e^{r}sim LN(mu_{r},sigma_{r})$$
Furthermore, by scaling $e^{r}$ by $R_{f}$ we arrive at:
$$R_{f},e^{r}sim LN(mu_{r}+text{ln}(R_{f}),sigma_{r})$$
Finally, we subtract the constant $R_{f}$ from the above term:
$$R_{f},e^{r}-R_{f}$$
Now, because the standard log-normal distribution is a 2-parameter distribution with support on $xin(0,infty)$, it needs to be adapted to account for the negative shift of $R_{f}$.
So, we now consider the 3-parameter log-normal distribution, which includes a location parameter, $theta$. Essentially, this adjusts the support of the distribution to be $xin(theta,infty)$. It has probability density function:
$$f_{X}(x;mu,sigma,theta)=frac{1}{(x-theta)sigmasqrt{2pi}}e^{frac{(text{ln}(x-theta)-mu)^{2}}{2sigma^{2}}}$$
where $x>theta,,sigma>0$. The mean and variance of the shifted log-normal distribution are easy enough to calculate. The mean is equal to the mean of the non-shifted log-normal plus the shift:
$$E[X+c]=E[X]+c$$
Similarly, the variance is equal to the variance of the non-shifted log-normal:
$$text{Var}(X+c)=text{Var}(X)$$
So we arrive at:
$$R=R_{f}(e^{r}-1)sim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
with probability density function:
$$f_{R}(r;mu,sigma,theta)=frac{1}{(r+R_{f})sigma_{r}sqrt{2pi}}e^{frac{big(text{ln}(r+R_{f})-mu_{r}-text{ln}(R_{f})big)^{2}}{2sigma_{r}^{2}}}$$
So to answer your question, for the equation:
$$R=c_{R}+epsilon_{R}$$
the value of $c_{R}$ is completely dependent on how you specify the parameters of $epsilon_{R}$. You can have:
$$c_{R}=0,,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
or
$$c_{R}=-R_{f},,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},0)$$
etc.
add a comment |
Using your notation, we have:
$$R=R_{f}(e^{r}-1)=R_{f},e^{r}-R_{f}$$
where
$$rsim N(mu_{r},sigma_{r})$$
Now, we also know that if $r$ has a normal distribution, then $e^{r}$ is log-normally distributed:
$$e^{r}sim LN(mu_{r},sigma_{r})$$
Furthermore, by scaling $e^{r}$ by $R_{f}$ we arrive at:
$$R_{f},e^{r}sim LN(mu_{r}+text{ln}(R_{f}),sigma_{r})$$
Finally, we subtract the constant $R_{f}$ from the above term:
$$R_{f},e^{r}-R_{f}$$
Now, because the standard log-normal distribution is a 2-parameter distribution with support on $xin(0,infty)$, it needs to be adapted to account for the negative shift of $R_{f}$.
So, we now consider the 3-parameter log-normal distribution, which includes a location parameter, $theta$. Essentially, this adjusts the support of the distribution to be $xin(theta,infty)$. It has probability density function:
$$f_{X}(x;mu,sigma,theta)=frac{1}{(x-theta)sigmasqrt{2pi}}e^{frac{(text{ln}(x-theta)-mu)^{2}}{2sigma^{2}}}$$
where $x>theta,,sigma>0$. The mean and variance of the shifted log-normal distribution are easy enough to calculate. The mean is equal to the mean of the non-shifted log-normal plus the shift:
$$E[X+c]=E[X]+c$$
Similarly, the variance is equal to the variance of the non-shifted log-normal:
$$text{Var}(X+c)=text{Var}(X)$$
So we arrive at:
$$R=R_{f}(e^{r}-1)sim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
with probability density function:
$$f_{R}(r;mu,sigma,theta)=frac{1}{(r+R_{f})sigma_{r}sqrt{2pi}}e^{frac{big(text{ln}(r+R_{f})-mu_{r}-text{ln}(R_{f})big)^{2}}{2sigma_{r}^{2}}}$$
So to answer your question, for the equation:
$$R=c_{R}+epsilon_{R}$$
the value of $c_{R}$ is completely dependent on how you specify the parameters of $epsilon_{R}$. You can have:
$$c_{R}=0,,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
or
$$c_{R}=-R_{f},,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},0)$$
etc.
add a comment |
Using your notation, we have:
$$R=R_{f}(e^{r}-1)=R_{f},e^{r}-R_{f}$$
where
$$rsim N(mu_{r},sigma_{r})$$
Now, we also know that if $r$ has a normal distribution, then $e^{r}$ is log-normally distributed:
$$e^{r}sim LN(mu_{r},sigma_{r})$$
Furthermore, by scaling $e^{r}$ by $R_{f}$ we arrive at:
$$R_{f},e^{r}sim LN(mu_{r}+text{ln}(R_{f}),sigma_{r})$$
Finally, we subtract the constant $R_{f}$ from the above term:
$$R_{f},e^{r}-R_{f}$$
Now, because the standard log-normal distribution is a 2-parameter distribution with support on $xin(0,infty)$, it needs to be adapted to account for the negative shift of $R_{f}$.
So, we now consider the 3-parameter log-normal distribution, which includes a location parameter, $theta$. Essentially, this adjusts the support of the distribution to be $xin(theta,infty)$. It has probability density function:
$$f_{X}(x;mu,sigma,theta)=frac{1}{(x-theta)sigmasqrt{2pi}}e^{frac{(text{ln}(x-theta)-mu)^{2}}{2sigma^{2}}}$$
where $x>theta,,sigma>0$. The mean and variance of the shifted log-normal distribution are easy enough to calculate. The mean is equal to the mean of the non-shifted log-normal plus the shift:
$$E[X+c]=E[X]+c$$
Similarly, the variance is equal to the variance of the non-shifted log-normal:
$$text{Var}(X+c)=text{Var}(X)$$
So we arrive at:
$$R=R_{f}(e^{r}-1)sim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
with probability density function:
$$f_{R}(r;mu,sigma,theta)=frac{1}{(r+R_{f})sigma_{r}sqrt{2pi}}e^{frac{big(text{ln}(r+R_{f})-mu_{r}-text{ln}(R_{f})big)^{2}}{2sigma_{r}^{2}}}$$
So to answer your question, for the equation:
$$R=c_{R}+epsilon_{R}$$
the value of $c_{R}$ is completely dependent on how you specify the parameters of $epsilon_{R}$. You can have:
$$c_{R}=0,,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
or
$$c_{R}=-R_{f},,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},0)$$
etc.
Using your notation, we have:
$$R=R_{f}(e^{r}-1)=R_{f},e^{r}-R_{f}$$
where
$$rsim N(mu_{r},sigma_{r})$$
Now, we also know that if $r$ has a normal distribution, then $e^{r}$ is log-normally distributed:
$$e^{r}sim LN(mu_{r},sigma_{r})$$
Furthermore, by scaling $e^{r}$ by $R_{f}$ we arrive at:
$$R_{f},e^{r}sim LN(mu_{r}+text{ln}(R_{f}),sigma_{r})$$
Finally, we subtract the constant $R_{f}$ from the above term:
$$R_{f},e^{r}-R_{f}$$
Now, because the standard log-normal distribution is a 2-parameter distribution with support on $xin(0,infty)$, it needs to be adapted to account for the negative shift of $R_{f}$.
So, we now consider the 3-parameter log-normal distribution, which includes a location parameter, $theta$. Essentially, this adjusts the support of the distribution to be $xin(theta,infty)$. It has probability density function:
$$f_{X}(x;mu,sigma,theta)=frac{1}{(x-theta)sigmasqrt{2pi}}e^{frac{(text{ln}(x-theta)-mu)^{2}}{2sigma^{2}}}$$
where $x>theta,,sigma>0$. The mean and variance of the shifted log-normal distribution are easy enough to calculate. The mean is equal to the mean of the non-shifted log-normal plus the shift:
$$E[X+c]=E[X]+c$$
Similarly, the variance is equal to the variance of the non-shifted log-normal:
$$text{Var}(X+c)=text{Var}(X)$$
So we arrive at:
$$R=R_{f}(e^{r}-1)sim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
with probability density function:
$$f_{R}(r;mu,sigma,theta)=frac{1}{(r+R_{f})sigma_{r}sqrt{2pi}}e^{frac{big(text{ln}(r+R_{f})-mu_{r}-text{ln}(R_{f})big)^{2}}{2sigma_{r}^{2}}}$$
So to answer your question, for the equation:
$$R=c_{R}+epsilon_{R}$$
the value of $c_{R}$ is completely dependent on how you specify the parameters of $epsilon_{R}$. You can have:
$$c_{R}=0,,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},-R_{f})$$
or
$$c_{R}=-R_{f},,,Rsim LN_{3}(mu_{r}+text{ln}(R_{f}),sigma_{r},0)$$
etc.
edited Aug 8 '17 at 5:27
answered Aug 7 '17 at 6:09
StatsPleaseStatsPlease
15817
15817
add a comment |
add a comment |
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