change_regime: Change the parameters of a specific regime of the given...

View source: R/parameterReforms.R

change_regimeR Documentation

Change the parameters of a specific regime of the given parameter vector

Description

change_regime changes the regime parameters (\phi_{m},vec(A_{m,1}),...,\vec(A_{m,p}),vech(\Omega_m)) (replace vech(\Omega_m) by vec(B_m) for cond_dist="ind_Student") of the given regime to the new given parameters.

Usage

change_regime(
  p,
  M,
  d,
  params,
  m,
  regime_pars,
  cond_dist = c("Gaussian", "Student", "ind_Student", "ind_skewed_t")
)

Arguments

p

the autoregressive order of the model

M

the number of regimes

d

the number of time series in the system, i.e., the dimension

params

a real valued vector specifying the parameter values. Should have the form \theta = (\phi_{1},...,\phi_{M},\varphi_1,...,\varphi_M,\sigma,\alpha,\nu), where (see exceptions below):

  • \phi_{m} = the (d \times 1) intercept (or mean) vector of the mth regime.

  • \varphi_m = (vec(A_{m,1}),...,vec(A_{m,p})) (pd^2 \times 1).

  • if cond_dist="Gaussian" or "Student":

    \sigma = (vech(\Omega_1),...,vech(\Omega_M)) (Md(d + 1)/2 \times 1).

    if cond_dist="ind_Student" or "ind_skewed_t":

    \sigma = (vec(B_1),...,vec(B_M) (Md^2 \times 1).

  • \alpha = the (a\times 1) vector containing the transition weight parameters (see below).

  • if cond_dist = "Gaussian"):

    Omit \nu from the parameter vector.

    if cond_dist="Student":

    \nu > 2 is the single degrees of freedom parameter.

    if cond_dist="ind_Student":

    \nu = (\nu_1,...,\nu_d) (d \times 1), \nu_i > 2.

    if cond_dist="ind_skewed_t":

    \nu = (\nu_1,...,\nu_d,\lambda_1,...,\lambda_d) (2d \times 1), \nu_i > 2 and \lambda_i \in (0, 1).

For models with...

weight_function="relative_dens":

\alpha = (\alpha_1,...,\alpha_{M-1}) (M - 1 \times 1), where \alpha_m (1\times 1), m=1,...,M-1 are the transition weight parameters.

weight_function="logistic":

\alpha = (c,\gamma) (2 \times 1), where c\in\mathbb{R} is the location parameter and \gamma >0 is the scale parameter.

weight_function="mlogit":

\alpha = (\gamma_1,...,\gamma_M) ((M-1)k\times 1), where \gamma_m (k\times 1), m=1,...,M-1 contains the multinomial logit-regression coefficients of the mth regime. Specifically, for switching variables with indices in I\subset\lbrace 1,...,d\rbrace, and with \tilde{p}\in\lbrace 1,...,p\rbrace lags included, \gamma_m contains the coefficients for the vector z_{t-1} = (1,\tilde{z}_{\min\lbrace I\rbrace},...,\tilde{z}_{\max\lbrace I\rbrace}), where \tilde{z}_{i} =(y_{it-1},...,y_{it-\tilde{p}}), i\in I. So k=1+|I|\tilde{p} where |I| denotes the number of elements in I.

weight_function="exponential":

\alpha = (c,\gamma) (2 \times 1), where c\in\mathbb{R} is the location parameter and \gamma >0 is the scale parameter.

weight_function="threshold":

\alpha = (r_1,...,r_{M-1}) (M-1 \times 1), where r_1,...,r_{M-1} are the threshold values.

weight_function="exogenous":

Omit \alpha from the parameter vector.

identification="heteroskedasticity":

\sigma = (vec(W),\lambda_2,...,\lambda_M), where W (d\times d) and \lambda_m (d\times 1), m=2,...,M, satisfy \Omega_1=WW' and \Omega_m=W\Lambda_mW', \Lambda_m=diag(\lambda_{m1},...,\lambda_{md}), \lambda_{mi}>0, m=2,...,M, i=1,...,d.

Above, \phi_{m} is the intercept parameter, A_{m,i} denotes the ith coefficient matrix of the mth regime, \Omega_{m} denotes the positive definite error term covariance matrix of the mth regime, and B_m is the invertible (d\times d) impact matrix of the mth regime. \nu_m is the degrees of freedom parameter of the mth regime. If parametrization=="mean", just replace each \phi_{m} with regimewise mean \mu_{m}.

m

which regime?

regime_pars
If cond_dist="Gaussian" or cond_dist="Student":

rhe (dp + pd^2 + d(d+1)/2) vector (\phi_{m},vec(A_{m,1}),...,\vec(A_{m,p}),vech(\Omega_m)).

If cond_dist="ind_Student" or "ind_skewed_t":

the (dp + pd^2 + d^2 + 1) vector (\phi_{m},vec(A_{m,1}),...,\vec(A_{m,p}),vec(B_m)).

Details

Does not support constrained models or structural models. Weight parameters and distribution parameters are not changed.

Value

Returns parameter vector with m:th regime changed to regime_pars.

References

  • Kheifets I.L., Saikkonen P.J. 2020. Stationarity and ergodicity of Vector STAR models. Econometric Reviews, 39:4, 407-414.

  • Lütkepohl H. 2005. New Introduction to Multiple Time Series Analysis, Springer.

  • Lanne M., Virolainen S. 2025. A Gaussian smooth transition vector autoregressive model: An application to the macroeconomic effects of severe weather shocks. Unpublished working paper, available as arXiv:2403.14216.

  • Virolainen S. 2025. Identification by non-Gaussianity in structural threshold and smooth transition vector autoregressive models. Unpublished working paper, available as arXiv:2404.19707.

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sstvars documentation built on April 11, 2025, 5:47 p.m.