The initial data of the problem ( b ≪ h) allow us to neglect the change in SSS components across the width b of the bar and to determine them using the system of static, physical, and geometrical equations of plane problem of the linear elasticity theory in the polar coordinate system:
$$ {\displaystyle \begin{array}{l}\frac{\partial {\sigma}_r}{\partial_r}+\frac{1}{r}\frac{\partial {\tau}_{r\theta}}{\partial \theta }+\frac{\sigma_r-{\sigma}_{\theta }}{r}=0\\ {}\frac{\partial {\tau}_{r\theta}}{\partial r}+\frac{1}{r}\frac{\partial {\sigma}_{\theta }}{\partial \theta }+\frac{2{\tau}_{\theta r}}{r}=0,\end{array}}\left\}{\displaystyle \begin{array}{l}{\varepsilon}_r=\frac{\sigma_r}{\mu_r^E}-\frac{\mu_{\theta r}^v{\sigma}_{\theta }}{\mu_{\theta}^E},\\ {}{\varepsilon}_{\theta }=\frac{\sigma_{\theta }}{\mu_{\theta}^E}-\frac{\mu_{r\theta}^v{\sigma}_r}{\mu_r^E},\\ {}{\gamma}_{r\theta}=\frac{1}{\mu_{r\theta}^G}{\tau}_{r\theta},\end{array}}\right\}{\displaystyle \begin{array}{l}{\varepsilon}_r=\frac{\partial {u}_r}{\partial r},\\ {}{\varepsilon}_{\theta }=\frac{1}{r}\left(\frac{\partial {\mu}_{\theta }}{\partial \theta }+{u}_r\right),\\ {}{\gamma}_{r\theta}=\frac{1}{r}\left(\frac{\partial {\mu}_r}{\partial \theta }-{u}_{\theta}\right)+\frac{\partial {\mu}_{\theta }}{\partial r}.\end{array}}\Big\} $$
(3)
According to the accepted system of external loads on the longitudinal surfaces Πϛ (ϛ = 1,2) and the end Τ1 of the bar, the static boundary conditions are
$$ {\displaystyle \begin{array}{l}{\left.{\sigma}_{\theta}\right|}_{\theta =0}=-{p}_{\theta}^{T_1},\\ {}{\left.{\sigma}_r\right|}_{r={r}_{\varsigma }}=0,\end{array}}\kern0.5em {\displaystyle \begin{array}{l}{\left.{\tau}_{\theta r}\right|}_{\theta =0}=-{p}_r^{T_1},\\ {}{\left.{\tau}_{r\theta}\right|}_{r={r}_{\varsigma }}=0.\end{array}} $$
(4)
Integrating the first and second relations of (4) over the cross section, with account of relations between the internal forces Nθ, Qr, and My and loads at the beam end, we arrive at the static conditions at the end Τ1
$$ {\displaystyle \begin{array}{c}b\underset{r_1}{\overset{r_2}{\int }}{\sigma}_{\theta }{\left|{}_{\theta =0} dr=b\underset{r_1}{\overset{r_2}{\int }}\left(-{p}_{\theta}^{T_1}\right) dr={N}_{\theta}\right|}_{\theta =0},\\ {}b\underset{r_1}{\overset{r_2}{\int }}{\tau}_{\theta r}{\left|{}_{\theta =0} dr=b\underset{r_1}{\overset{r_2}{\int }}\left(-{p}_r^{T_1}\right) dr={Q}_r\right|}_{\theta =0},\\ {}{\left.b\underset{r_1}{\overset{r_2}{\int }}\Big[{\sigma}_{\theta}\right|}_{\theta =0}\left(r-{r}_C\right)\left] dr=b\underset{r_1}{\overset{r_2}{\int }}\right[-{p}_r^{T_1}\Big(r-{\left|{r}_C\left)\right] dr={M}_y\right|}_{\theta =0}.\end{array}} $$
(5)
Solving static equations (3) for the normal stresses, with account of boundary conditions (4) on the longitudinal sides and paired shear stresses, we have
$$ {\displaystyle \begin{array}{c}{\sigma}_r=-\frac{1}{r}\underset{r_1}{\overset{r}{\int }}\left({\left.\frac{\partial {\tau}_{r\theta}}{\partial r} d\theta +2\underset{0}{\overset{\theta }{\int }}{\tau}_{r\theta} d\theta -{\sigma}_{\theta}\right|}_{\theta =0}\right) d r,\\ {}{\left.{\sigma}_{\theta }=-\underset{0}{\overset{\theta }{\int }}\left(r\frac{\partial {\tau}_{r\theta}}{\partial r}+2{\tau}_{\theta r}\right) d\theta +{\sigma}_{\theta}\right|}_{\theta =0}.\end{array}} $$
(6)
An approximate form of solutions for the shear stresses τrθ in (6) can be found from the distribution of the transverse force Qr, which, for the bar considered, can be written as follows:
$$ {Q}_r=-b\left(\sin \theta \underset{r_1}{\overset{r_2}{\int }}{p}_{\theta}^{{\mathrm{T}}_1} dr+\cos \theta \underset{r_1}{\overset{r_2}{\int }}{p}_r^{{\mathrm{T}}_1} dr\right)=b\underset{r_1}{\overset{r_2}{\int }}{\tau}_{\theta r} dr. $$
(7)
According to relation (7), the possible form of solution for the shear stresses τrθ is
$$ {\tau}_{r\theta}={R}_{r\theta}^{\tau 1}\sin \theta +{R}_{r\theta}^{\tau 2}\cos \theta, $$
(8)
where \( {R}_{r\theta}^{\tau 1}={R}_{r\theta}^{\tau 1}(r) \) and \( {R}_{r\theta}^{\tau 2}={R}_{r\theta}^{\tau 2}(r) \) are unknown distribution functions of shear stresses along the height of cross section.
Inserting Eq. (8) into the fourth boundary condition of (4) and considering that it has to be satisfied for all points of the longitudinal surfaces Πϛ, we arrive at the following boundary conditions for the functions \( {R}_{r\theta}^{\tau 1} \) and \( {R}_{r\theta}^{\tau 2} \):
$$ {R}_{r\theta}^{\tau 1}{\left|{}_{r={r}_{\varsigma }}=0,\kern1em {R}_{r\theta}^{\tau 2}\right|}_{r={r}_{\varsigma }}=0. $$
(9)
Inserting Eq. (8) into solutions (6), after some transformations with account of Eqs. (9), we have
$$ {\displaystyle \begin{array}{c}{\sigma}_r={R}_{r\theta}^{\tau 1}\cos \theta -{R}_{r\theta}^{\tau 2}\sin \theta +{R}_r^{\sigma },\\ {}{\sigma}_{\theta }=\frac{1}{r}\frac{d}{dr}\left({r}^2{R}_{r\theta}^{\tau 1}\cos \theta -{r}^2{R}_{r\theta}^{\tau 2}\sin \theta \right)+\frac{d}{dr}\left(r{R}_r^{\sigma}\right),\end{array}} $$
(10)
where
$$ {\left.{R}_r^{\sigma }=-{R}_{r\theta}^{\tau 1}-\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{R}_{r\theta}^{\tau 1} dr+\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{\sigma}_{\theta}\right|}_{\theta =0} dr. $$
(11)
Inserting the second relation of (10) into the third boundary condition of (4), after transformations with account of Eqs. (9), we find boundary conditions for the function \( {R}_r^{\sigma } \):
$$ {\left.{R}_r^{\sigma}\right|}_{r={r}_{\varsigma }}=0,\kern1em \zeta =1,2. $$
(12)
Using integral conditions (5), together with Eqs. (8) and (11), the following conditions for the unknown functions are obtained:
$$ {\displaystyle \begin{array}{c}\underset{r_1}{\overset{r_2}{\int }}{R}_{r\theta}^{\tau 1} dr=\frac{1}{b}{N}_{\theta }{\left|{}_{\theta =0},\kern1em \underset{r_1}{\overset{r_2}{\int }}{R}_{r\theta}^{\tau 2} dr=\frac{1}{b}{Q}_r\right|}_{\theta =0},\\ {}\underset{r_1}{\overset{r_2}{\int }}\left(r{R}_r^{\sigma}\right) dr=-\frac{1}{b}\left({r}_C{N}_{\theta }{\left|{}_{\theta =0}+{M}_y\right|}_{\theta =0}\right).\end{array}} $$
(13)
Thus, the further solution of the problem consists in determination of functions \( {R}_{r\theta}^{\tau 1} \), \( {R}_{r\theta}^{\tau 2} \), and \( {R}_r^{\sigma } \), agreeing with boundary and integral conditions (9), (12), and (13). To determine these functions, we use the remaining equations of (3).
Solving the first and second geometrical relations of (3) for the displacements ur and uθ, we have
$$ {\left.{u}_r=\underset{r_1}{\overset{r}{\int }}{\varepsilon}_r dr+{u}_r\right|}_{r={r}_1},\kern1em {u}_{\theta }=r\underset{0}{\overset{\theta }{\int }}{\varepsilon}_{\theta } d\theta -\underset{0}{\overset{\theta }{\int }}\underset{r_1}{\overset{r}{\int }}{\varepsilon}_r dr d\theta -\underset{0}{\overset{\theta }{\int }}{u}_r{\left|{}_{r={r}_1} d\theta +{u}_{\theta}\right|}_{\theta =0}. $$
(14)
Inserting Eqs. (14) into the last geometrical relation of (3), leads to the compatibility conditions for strains and displacements
$$ {\displaystyle \begin{array}{c}{r}^2\underset{0}{\overset{\theta }{\int }}\frac{\partial {\varepsilon}_{\theta }}{\partial r} d\theta +\underset{r_1}{\overset{r}{\int }}\frac{\partial {\varepsilon}_r}{\partial \theta } d r+\underset{0}{\overset{\theta }{\int }}\underset{r_1}{\overset{r}{\int }}{\varepsilon}_r d r d\theta -r\underset{0}{\overset{\theta }{\int }}{\varepsilon}_r d\theta \\ {}+\frac{{\left.d{u}_r\right|}_{r={r}_1}}{d\theta}+\underset{0}{\overset{\theta }{\int }}{u}_r{\left|{}_{r={r}_1} d\theta +r\frac{{\left.d{u}_{\theta}\right|}_{\theta =0}}{d r}-{u}_{\theta}\right|}_{\theta =0}=r{\gamma}_{r\theta}.\end{array}} $$
(15)
Expression (15) is the governing equation for solving the problem considered. To put it into a final form, physical relations (3) and the preliminary solutions (8) and (10) for stresses are employed.
Inserting Eqs. (8) and (10) into physical relations (3) leads to relations for the linear and shear strains in the form
$$ {\displaystyle \begin{array}{c}{\varepsilon}_r={R}_r^{\varepsilon 1}\cos \theta +{R}_r^{\varepsilon 2}\sin \theta +{R}_r^{\varepsilon 3},\kern1.1em {\varepsilon}_{\theta }={R}_{\theta}^{\varepsilon 1}\cos \theta +{R}_{\theta}^{\varepsilon 2}\sin \theta +{R}_{\theta}^{\varepsilon 3},\\ {}{\gamma}_{r\theta}=\frac{R_{r\theta}^{\tau 1}\sin \theta }{\mu_{r\theta}^G}+\frac{R_{r\theta}^{\tau 2}\cos \theta }{\mu_{r\theta}^G},\end{array}} $$
(16)
where the following designations for the components of distribution of the linear strains along the height of bar cross section have been introduced:
$$ {\displaystyle \begin{array}{c}{R}_r^{\varepsilon 1}=-\frac{\mu_{\theta r}^v}{\mu_{\theta}^E}\frac{1}{r}\frac{d\left({r}^2{R}_{r\theta}^{\tau 1}\right)}{dr}+\frac{R_{r\theta}^{\tau 1}}{\mu_{\theta}^E},\kern1em {R}_r^{\varepsilon 2}=\frac{\mu_{\theta r}^v}{\mu_{\theta}^E}\frac{1}{r}\frac{d\left({r}^2{R}_{r\theta}^{\tau 2}\right)}{dr}-\frac{R_{r\theta}^{\tau 2}}{\mu_r^E},\\ {}{R}_r^{\varepsilon 3}=-\frac{\mu_{\theta r}^v}{\mu_{\theta}^E}\frac{1}{r}\frac{d\left(r{R}_r^{\sigma}\right)}{dr}+\frac{1}{\mu_r^E}{R}_r^{\sigma },\kern1em {R}_{\theta}^{\varepsilon 1}=\frac{1}{\mu_{\theta}^E}\frac{1}{r}\frac{d\left({r}^2{R}_{r\theta}^{\tau 1}\right)}{dr}-\frac{\mu_{r\theta}^v{R}_{r\theta}^{\tau 1}}{\mu_r^E},\\ {}{R}_{\theta}^{\varepsilon 2}=-\frac{1}{\mu_{\theta}^E}\frac{1}{r}\frac{d\left({r}^2{R}_{r\theta}^{\tau 2}\right)}{dr}+\frac{\mu_{r\theta}^v{R}_{r\theta}^{\tau 2}}{\mu_r^E},\kern1em {R}_{\theta}^{\varepsilon 2}=\frac{1}{\mu_{\theta}^E}\frac{d\left({r}^2{R}_r^{\sigma}\right)}{dr}-\frac{\mu_{r\theta}^v}{\mu_r^E}{R}_r^{\sigma }.\end{array}} $$
Inserting relations (16) into Eq. (15) and performing necessary transformations, we obtain the integrodifferential equation
$$ {\displaystyle \begin{array}{c}\left[{r}^2\frac{d{R}_{\theta}^{\varepsilon 1}}{d r}-r{R}_r^{\varepsilon 1}-\frac{r{R}_{r\theta}^{\tau 1}}{\mu_{r\theta}^G}\right]\sin \theta -\left[{r}^2\frac{d{R}_{\theta}^{\varepsilon 2}}{d r}-r{R}_r^{\varepsilon 2}-\frac{r{R}_{r\theta}^{\tau 2}}{\mu_{r\theta}^G}\right]\cos \theta \\ {}+\left[{r}^2\frac{d}{d r}\left({R}_{\theta}^{\varepsilon 3}-\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 3} d r\right)\right]\theta -\left[{r}^2\frac{d}{d r}\left(-\frac{{\left.{u}_{\theta}\right|}_{\theta =0}}{r}-{R}_{\theta}^{\varepsilon 2}+\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 3} d r\right)\right]\\ {}{\left.+\frac{{\left.d{u}_r\right|}_{r={r}_1}}{d\theta}+\underset{0}{\overset{\theta }{\int }}{u}_r\right|}_{r={r}_1} d\theta =0.\end{array}} $$
(18)
A nontrivial solution of Eq. (18) for the unknown functions is possible only if the expressions in square brackets in it are equal to some constants:
$$ {\displaystyle \begin{array}{c}{r}^2\frac{d{R}_{\theta}^{\varepsilon 1}}{dr}-r{R}_r^{\varepsilon 1}-\frac{r{R}_{r\theta}^{\varepsilon 1}}{\mu_{r\theta}^G}={K}_1,\kern1em {r}^2\frac{d{R}_{\theta}^{\varepsilon 2}}{dr}-r{R}_r^{\varepsilon 2}+\frac{r{R}_{r\theta}^{\varepsilon 2}}{\mu_{r\theta}^G}={K}_2,\\ {}{r}^2\frac{d}{dr}\left({R}_{\theta}^{\varepsilon 3}-\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 3} dr\right)={K}_3,\kern1em {r}^2\frac{d}{dr}\left(-\frac{{\left.{u}_{\theta}\right|}_{\theta =0}}{r}-{R}_{\theta}^{\varepsilon 2}+\frac{1}{r}\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 3} dr\right)={K}_4.\end{array}} $$
(19)
With account of Eqs. (19), Eq. (18) takes the form
$$ {\left.\frac{{\left.d{u}_r\right|}_{r={r}_1}}{d\theta}+\underset{0}{\overset{\theta }{\int }}{u}_r\right|}_{r={r}_1}\; d\theta =-{K}_1\sin \theta +{K}_2\cos \theta -{K}_3\theta +{K}_4. $$
(20)
Thus, the further solution of the problem is reduced to the search for solutions of the ordinary differential equations (19) and (20). Let us consider the basic approaches to finding the general and particular solutions of the given equations.
Inserting relations (17) into the first equation of (19), we arrive at the governing equation for the function \( {R}_{r\theta}^{\tau 1} \) in the form
$$ {\displaystyle \begin{array}{c}r\frac{d}{dr}\left[\frac{r}{\mu_{\theta}^E}\frac{d{R}_{r\theta}^{\tau 1}}{dr}+\left(\frac{2}{\mu_{\theta}^E}-\frac{\mu_{r\theta}^v}{\mu_r^E}\right){R}_{r\theta}^{\tau 1}\right]\\ {}+\frac{\mu_{\theta r}^v}{\mu_{\theta}^E}r\frac{d{R}_{r\theta}^{\tau 1}}{dr}+\left(\frac{2{\mu}_{\theta r}^v}{\mu_{\theta}^E}-\frac{1}{\mu_r^E}-\frac{1}{\mu_{r\theta}^G}\right){R}_{r\theta}^{\tau 1}=\frac{K_1}{r}.\end{array}} $$
(21)
Equation (21) is a homogeneous differential equation with coefficients varying stepwise on the borders of layers of the bar. Within the limits of a kth homogeneous layer at r ∈ (rdb, k − 1, rdb, k) , the given equation is transformed into a special form of the Cauchy–Euler, namely,
$$ {r}^2\frac{d^2{R_{r\theta}^{\tau 1}}^{\left[k\right]}}{d{r}^2}+{\alpha}_1^{\left[k\right]}r\frac{d{R_{r\theta}^{\tau 1}}^{\left[k\right]}}{dr}+{\alpha}_0^{\left[k\right]}{R_{r\theta}^{\tau 1}}^{\left[k\right]}=\frac{K_1{E}_{\theta}^{\left[k\right]}}{r},k=\overline{1,m}, $$
(22)
where
$$ {\displaystyle \begin{array}{cc}{\alpha}_0^{\left[k\right]}=2{\nu}_{\theta r}^{\left[k\right]}-\frac{E_{\theta}^{\left[k\right]}}{E_r^{\left[k\right]}}-\frac{E_{\theta}^{\left[k\right]}}{G_{r\theta}^{\left[k\right]}},& {\alpha}_1^{\left[k\right]}=3+{\nu}_{\theta r}^{\left[k\right]}-\frac{E_{\theta}^{\left[k\right]}{\nu}_{r\theta}^{\left[k\right]}}{E_r^{\left[k\right]}}.\end{array}} $$
(23)
The general solution of Eq. (22) is
$$ {R}_{r\theta}^{\tau 1\left[k\right]}={C}_{11}^{\left[k\right]}{r}^{\kappa_1^{\left[k\right]}}+{C}_{21}^{\left[k\right]}{r}^{\kappa_2^{\left[k\right]}}+\frac{K_1{E}_{\theta}^{\left[k\right]}}{\alpha_0^{\left[k\right]}-{\alpha}_1^{\left[k\right]}+2}\frac{1}{r},k=\overline{1,m}, $$
(24)
where \( {C}_{11}^{\left[k\right]} \) and \( {C}_{21}^{\left[k\right]} \)[ ] are unknown constants of integration; \( {\kappa}_1^{\left[k\right]} \) and \( {\kappa}_2^{\left[k\right]} \) are roots of the characteristic equation
$$ {\kappa}_{1,2}^{\left[k\right]}=\frac{1}{2}\left(1-{\alpha}_1^{\left[k\right]}\pm \sqrt{{\left({\alpha}_1^{\left[k\right]}-1\right)}^2-4{\alpha}_0^{\left[k\right]}}\right). $$
(25)
We should note that, for the case of an isotropic layer, where \( {E}_r^{\left[k\right]}={E}_{\theta}^{\left[k\right]}={E}^{\left[k\right]} \), \( {\nu}_{r\theta}^{\left[k\right]}={\nu}_{\theta r}^{\left[k\right]}={\nu}^{\left[k\right]} \), and \( {G}_{r\theta}^{\left[k\right]}={G}^{\left[k\right]}={E}^{\left[k\right]}/\left(2+2{\nu}^{\left[k\right]}\right) \), solution (24) is transformed to
$$ {R}_{r\theta}^{\tau 1\left[k\right]}={C}_{11}^{\left[k\right]}r+{C}_{21}^{\left[k\right]}\frac{1}{r^3}-\frac{K_1{E}^{\left[k\right]}}{4}\frac{1}{r}. $$
(26)
The function \( {R}_{r\theta}^{\tau 1} \) for all the bar can be collected from solutions (24) in the same way as the functions of elastic constants (2):
$$ {R}_{r\theta}^{\tau 1}=\sum \limits_{k=1}^m{R}_{r\theta}^{\tau 1\left[k\right]}\left[H\left(r-{r}_{bd,k-1}\right)-H\left(r-{r}_{bd,k}\right)\right]. $$
(27)
Similarly to Eq. (21), the second equation of (19), with account of Eqs. (17), takes the following form within the limits of a kth layer:
$$ {r}^2\frac{d^2{R}_{r\theta}^{\tau 2\left[k\right]}}{d{r}^2}+{\alpha}_1^{\left[k\right]}r\frac{d{R}_{r\theta}^{\tau 2\left[k\right]}}{dr}={\alpha}_0^{\left[k\right]}{R}_{r\theta}^{\tau 2\left[k\right]}=-\frac{K_2{E}_{\theta}^{\left[k\right]}}{r},k=\overline{1,m}. $$
(28)
The general solution of Eq. (28) is similar to solutions (24) and (26) for orthotropic and isotropic layers, respectively:
$$ {R}_{r\theta}^{\tau 2\left[k\right]}={C}_{12}^{\left[k\right]}{r}^{\kappa_1^{\left[k\right]}}+{C}_{22}^{\left[k\right]}{r}^{\kappa_2^{\left[k\right]}}-\frac{K_2{E}_{\theta}^{\left[k\right]}}{\alpha_0^{\left[k\right]}-{\alpha}_1^{\left[k\right]}+2}\frac{1}{r},\kern0.36em k=\overline{1,m}, $$
(29)
$$ {R}_{r\theta}^{\tau 2\left[k\right]}={C}_{12}^{\left[k\right]}r+{C}_{22}^{\left[k\right]}\frac{1}{r^3}+\frac{K_2{E}^{\left[k\right]}}{4}\frac{1}{r},\kern0.36em k=\overline{1,m}, $$
(30)
For all the package of layers, the solution is written in the form
$$ {R}_{r\theta}^{\tau 2}=\sum \limits_{k=1}^m{R}_{r\theta}^{\tau 2\left[k\right]}\left[H\left(r-{r}_{bd,k-1}\right)-H\left(r-{r}_{bd,k}\right)\right]. $$
(31)
We should note that the function \( {R}_{r\theta}^{\tau 2} \) determines the stress components caused by the tangential load. As can be seen, in solution (30) for an isotropic layer, the fundamental system is similar to the solution of the problem on bending of an isotropic circular bar by a transverse force [16]. To some part, this confirms the validity of the solution construc ted.
Integrating the third equation of (19), we have
$$ r{R}_{\theta}^{\varepsilon 3}-\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 3} dr=-{K}_3+r{K}_5. $$
(32)
We transform Eq. (32) to the form
$$ {\left.r\left({R}_{\theta}^{\varepsilon 3}-{K}_5\right)-\int {R}_r^{\varepsilon 3} dr=-\Big({K}_3+\left(\int {R}_r^{\varepsilon 3} dr\right)\right|}_{r={r}_1}\Big)=\mathrm{const}. $$
(33)
Integrodifferential equation (33) with account of Eqs. (17) can have a solution only if \( {\left.{K}_3+\left(\int {R}_r^{\varepsilon 3} dr\right)\right|}_{r={r}_1} \) whence
$$ {\left.{K}_3=-\frac{1}{E_r^{\left[1\right]}}\left(\int {R}_r^{\sigma } dr\right)\right|}_{r={r}_1}. $$
(34)
Inserting Eqs. (17) into Eq. (32) with account of Eq. (34), it becomes
$$ r\left(\frac{1}{\mu_{\theta}^E}\frac{d}{dr}\left(r{R}_r^{\sigma}\right)-\frac{\mu_{r\theta}^{\nu }}{\mu_r^E}{R}_r^{\sigma}\right)-\int \left(\frac{1}{\mu_r^E}{R}_r^{\sigma }-\frac{\mu_{\theta r}^{\nu }}{\mu_{\theta}^E}\frac{d}{dr}\left(r{R}_r^{\sigma}\right)\right)\; dr={K}_5r. $$
(35)
Differentiating Eq. (35), we obtain a linear differential equation that, within the limits of any kth layer, take the form
$$ {r}^2\frac{d^2}{d{r}^2}\left(r{R}_r^{\sigma \left[k\right]}\right)+{\beta}_1^{\left[k\right]}r\frac{d}{dr}\left(r{R}_r^{\sigma \left[k\right]}\right)+{\beta}_0^{\left[k\right]}\left(r{R}_r^{\sigma \left[k\right]}\right)={K}_5{E}_{\theta}^{\left[k\right]}r,k=\overline{1,m}, $$
(36)
where
$$ {\displaystyle \begin{array}{cc}{\beta}_0^{\left[k\right]}=-\frac{E_{\theta}^{\left[k\right]}}{E_r^{\left[k\right]}},& {\beta}_1^{\left[k\right]}=1+{\nu}_{\theta r}^{\left[k\right]}\frac{E_{\theta}^{\left[k\right]}{\nu}_{r\theta}^{\left[k\right]}}{E_r^{\left[k\right]}}.\end{array}} $$
(37)
The general solution of Eq. (36) is found to be
$$ {R}_r^{\sigma \left[k\right]}={C}_{13}^{\left[k\right]}{r}^{\kappa_3^{\left[k\right]}-1}+{C}_{23}^{\left[k\right]}{r}^{\kappa_4^{\left[k\right]}-1}+\frac{K_5{E}_{\theta}^{\left[k\right]}}{\beta_0^{\left[k\right]}+{\beta}_1^{\left[k\right]}},\kern0.36em k=\overline{1,m}, $$
(38)
where \( {\kappa}_3^{\left[k\right]} \) and \( {\kappa}_4^{\left[k\right]} \) are roots of the characteristic equation
$$ {\kappa}_{3,4}^{\left[k\right]}=\frac{1}{2}\left[1-{\beta}_3^{\left[k\right]}\pm \sqrt{{\left({\beta}_1^{\left[k\right]}-1\right)}^2-4{\beta}_0^{\left[k\right]}}\right]. $$
(39)
We should note that, for an isotropic layer, the form of the solution varies, as \( {\beta}_{0,1}^{\left[k\right]}=\mp 1 \) in this case, to which there corresponds the solution
$$ {R}_r^{\sigma \left[k\right]}={C}_{13}^{\left[k\right]}+{C}_{23}^{\left[k\right]}\frac{1}{r^2}+\frac{K_5{E}_{\theta}^{\left[k\right]}}{2}\ln r. $$
(40)
According to Eqs. (10) and (13), the function \( {R}_r^{\sigma } \) is a component of distribution of the normal stresses σθ and σr caused by the resultant of moment of the normal load at the beam end Τ1. By the corresponding transformations (10) and (40) the known Golovin solution for the pure bending of a circular bar [16] can be obtained, which once again indirectly confirms the validity of the solution found.
For all the bar, the solution for the function \( {R}_r^{\sigma } \) is similar to (27):
$$ {R}_r^{\sigma }=\sum \limits_{k=1}^m{R}_r^{\sigma \left[k\right]}\left[H\left(r-{r}_{bd,k-1}\right)-H\left(r-{r}_{bd,k}\right)\right]. $$
(41)
We should note that Eqs. (19) also remain unchanged in the case where layer materials are continuously inhomogeneous in the radial direction: \( {S}_a^{\left[k\right]}={S}_a^{\left[k\right]}(r) \). However, in this case, their solutions in a finite form can be obtained only in special cases of \( {S}_a^{\left[k\right]}(r) \), which, with reference to a homogeneous circular bar are considered in [10].
The solution of the last equation of (19) can be found for all the package of bar layers by a direct integration. With the use of Eqs. (17), the solution of the given equation takes the form
$$ {\left.{u}_{\theta}\right|}_{\theta =0}=-r{R}_{\theta}^{\varepsilon 2}+\underset{r_1}{\overset{r}{\int }}{R}_r^{\varepsilon 2} dr+r{K}_6+{K}_4. $$
(42)
To solve Eq. (20), we introduce the replacement
$$ {\left.\underset{0}{\overset{\theta }{\int }}{u}_r\right|}_{r={r}_1} d\theta ={R}^u, $$
(43)
and Eq. (20) becomes
$$ \frac{d{R}^u}{d\theta}+{R}^u=-{K}_1\sin \theta +{K}_2\cos \theta -{K}_3\theta +{K}_4. $$
(44)
We should note that replacement (43) suggested the natural condition Ru|θ = 0 = 0 for the function Ru, in view of which the general solution of Eq. (44) is
$$ {R}^u=\frac{1}{2}{K}_1\theta \cos \theta +\frac{1}{2}{K}_2\theta \sin \theta -{K}_3\theta +{K}_4\left(1-\cos \theta \right)+{K}_7\sin \theta . $$
(45)
Differentiating Eq. (45) with account of Eqs. (43) and (34) leads to the relation
$$ {\displaystyle \begin{array}{c}{\left.{u}_r\right|}_{r={r}_1}=\frac{1}{2}{K}_1\left(\cos \theta -\theta \sin \theta \right)+\frac{1}{2}{K}_2\left(\cos \theta +\theta \sin \theta \right)\\ {}{\left.+\frac{1}{E_r^{\left[k\right]}}\left(\int {R}_r^{\sigma \left[1\right]} dr\right)\right|}_{r={r}_1}+{K}_4\sin \theta +{K}_7\cos \theta .\end{array}} $$
(46)
Thus, the general solutions for all the unknown functions \( {\left.{R}_{r\theta}^{\tau 1},{R}_{r\theta}^{\tau 2},{R}_r^{\sigma },{u}_{\theta}\right|}_{\theta =0} \), and \( {\left.{u}_r\right|}_{r={r}_1} \) of the problem considered have been found. These solutions, together with Eqs. (8), (10), (14), (16), and (17), allow one to determine relations for all SSS components of the multilayer bar considered. However, they will contain 6m+ 6 unknown constants of integration. A part of them can be found from boundary conditions (9) and (12) and integral conditions (13). The others are determined from the condition of absolutely rigid contact between layers and kinematic conditions at the fixed bar end.
$$ {\displaystyle \begin{array}{c}\begin{array}{cc}{R}_{r\theta}^{\tau 1\left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_{r\theta}^{\tau 1\left[k+1\right]}\right|}_{r={r}_{db,k}},& {R}_{r\theta}^{\tau 2\left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_{r\theta}^{\tau 2\left[k+1\right]}\right|}_{r={r}_{db,k}},\end{array}\\ {}{R}_r^{\sigma \left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_r^{\sigma \left[k+1\right]}\right|}_{r={r}_{db,k}},k=\overline{1,m-1}.\end{array}} $$
(47)
We require that the displacements ur and uθ also be continuous on the interfaces of layers Pk. According to the first ratio of (14), the solution for ur is continuous at any values of unknown constants in the solutions for \( {R}_{r\theta}^{\tau 1},{R}_{r\theta}^{\tau 2} \), and \( {R}_r^{\sigma } \), and the solution for uθ, in view of the last equation of (19), is continuous if continuous are εθ and \( {\left.{u}_{\theta}\right|}_{u_{\theta }=0} \) :
$$ {\varepsilon}_{\theta}^{\left[k\right]}{\left|{}_{r={r}_{db,k}}={\varepsilon}_{\theta}^{\left[k+1\right]}\right|}_{r={r}_{db,k}},k=\overline{1,m-1} $$
(48)
Inserting Eqs.(16) into Eqs. (48) and comparing the coefficient of identical functions of θ, it was established that
$$ {\displaystyle \begin{array}{c}\begin{array}{cc}{R}_{\theta}^{\varepsilon 1\left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_{\theta}^{\varepsilon 1\left[k+1\right]}\right|}_{r={r}_{db,k}},& {R}_{\theta}^{\varepsilon 2\left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_{\theta}^{\varepsilon 2\left[k+1\right]}\right|}_{r={r}_{db,k}},\end{array}\\ {}{R}_{\theta}^{\varepsilon 3\left[k\right]}{\left|{}_{r={r}_{db,k}}={R}_{\theta}^{\varepsilon 3\left[k+1\right]}\right|}_{r={r}_{db,k}},k=\overline{1,m-1}.\end{array}} $$
(49)
According to Eq. (42), continuity of the function \( {\left.{u}_{\theta}\right|}_{u_{\theta }=0} \) is fulfilled automatically if condition (49) holds.
Solutions (24) and (29), together with conditions (9), (47), and (49) and relations (17), show that the functions \( {R}_{r\theta}^{\tau 1} \) and \( {R}_{r\theta}^{\tau 2} \) are linearly dependent, i.e.,
$$ {R}_{r\theta}^{\tau 1}=\psi {R}_{r\theta}^{\tau 2}, $$
(50)
where ψ is a constant.
Applying Eq. (50) to the first two integral conditions (13), we have
$$ \psi ={Q}_r{\left|{}_{\theta =0}/{N}_{\theta}\right|}_{\theta =0}. $$
(51)
Relations (50) and (51) reduce the number of unknown constants by one third, to 4m+ 5 . As a result, only one of the functions \( {R}_{r\theta}^{\tau 1} \) and \( {R}_{r\theta}^{\tau 2} \) has to be determined. However, it is necessary to take into account some loading cases at which Eq. (50) loses its meaning:
-
if Nθ|θ = 0 = 0, then \( \psi =\infty \Rightarrow {R}_{r\theta}^{\tau 1}=0\wedge {R}_{r\theta}^{\tau 2}\ne 0 \);
-
if Qr|θ = 0 = Nθ|θ = 0 = 0, then \( \psi =0/0\Rightarrow {R}_{r\theta}^{\tau 1}={R}_{r\theta}^{\tau 2}\ne 0 \).
Conditions (9), (12), (13), (47), and (49), with account of Eqs. (50) and (51), allow one to find all unknown constants for the functions \( {R}_{r\theta}^{\tau 1},{R}_{r\theta}^{\tau 2} \), and \( {R}_r^{\sigma } \). The remaining constants K4,K6, and K7 are determined from the kinematic conditions at the beam end Τ2.
For the case considered, where the work of the circular cantilever is modeled, the fastening can be ensured forbidding circumferential displacements uθ for two points of the end Τ2 and the radial displacement ur of one of its points (Fig. 2), for example,
$$ {\displaystyle \begin{array}{ccc}{\left.{u}_r\right|}_{\theta ={\theta}_2,r={r}_1}=\mid 0,& {\left.{u}_{\theta}\right|}_{\theta ={\theta}_2,r={r}_1}=\mid 0,& {\left.{u}_{\theta}\right|}_{\theta ={\theta}_2,r={r}_2}=\mid 0,\end{array}} $$
(52)
From the viewpoint of static conditions, possible are also other combination of fixed points of the end or the longitudinal sides, but their analysis is already the subject of investigation of applied applications of the solution found.
Thus, we have obtained a system of analytical relations (8), (10), (14), (16), (17), (24), (27), (29), (31), (38), (41), (42), and (46) and conditions (9), (12), (13), (47), (49), (50), (51), and (52) that allows one to determine all SSS components for the problem on bending of a circular multilayer bar by normal and tangential loads at its ends. This solution is exact for the corresponding plane problem of elasticity theory, provided that the loads on the end Τ1 are distributed according to the relations found, namely,
$$ {\displaystyle \begin{array}{cc}{p}_{\theta}^{{\mathrm{T}}_1}=-\left[\frac{1}{r}\frac{d}{dr}\left({r}^2{R}_{r\theta}^{\tau 1}\right)+\frac{d}{dr}\left(r{R}_r^{\sigma}\right)\right],& {p}_r^{{\mathrm{T}}_1}={R}_{r\theta}^{\tau 2}\end{array}} $$
(53)
For other types of load distribution, according to the Saint Venant principle, the solution of the problem will differ from the exact decision only the on a small distance from the loaded bar end.
The relations obtained for SSS components become considerably simpler if layer materials are not compliant to the strains of transverse shear and compression, \( {E}_r^{\left[k\right]},{G}_{r\theta}^{\left[k\right]}\to \infty \), \( {\nu}_{r\theta}^{\left[k\right]},{\nu}_{\theta r}^{\left[k\right]}\to 0 \), \( k=\overline{1,m} \), which corresponds to the hypothesis of plane cross sections of the engineering theory of bending. In that case, solutions for the governing functions \( {R}_{r\theta}^{\tau 1},{R}_{r\theta}^{\tau 2} \), and Rr σ with account of boundary conditions (9) and (12) and integral conditions (13), take the form
$$ {\displaystyle \begin{array}{c}{R}_{r\theta}^{\tau 1}=-\frac{F_{\theta }}{b{D}_{-1}}\frac{1}{r^2}\left(\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr-\frac{B_0}{B_1}\underset{r_1}{\overset{r}{\int }}\left({\mu}_{\theta}^Er\right) dr\right),\\ {}{R}_{r\theta}^{\tau 2}=-\frac{F_r}{b{D}_{-1}}\frac{1}{r^2}\left(\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr-\frac{B_0}{B_1}\underset{r_1}{\overset{r}{\int }}\left({\mu}_{\theta}^Er\right) dr\right),\\ {}{R}_r^{\sigma }=-\frac{r_C{F}_{\theta }+M}{b{D}_0}\frac{1}{r}\left(\underset{r_1}{\overset{r}{\int }}\frac{\mu_{\theta}^E}{r} dr-\frac{B_{-1}}{B_0}\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr\right),\\ {}{\left.{u}_{\theta}\right|}_{\theta =0}=-\frac{F_r}{b{D}_{-1}}\left(1-\frac{B_0}{B_r}r\right)+{K}_4-{C}_7r,\\ {}{\left.{u}_r\right|}_{r={r}_1}=\frac{F_{\theta}\left(\cos \theta -\sin \theta \right)}{2b{D}_{-1}}-\frac{F_{\theta}\left(\theta \cos \theta +\sin \theta \right)}{2b{D}_{-1}}-\frac{r_C{F}_{\theta }+M}{b{D}_0}+{K}_4\sin \theta +{K}_7\cos \theta, \end{array}} $$
(54)
where Fr, Fθ, and M are resultant of the loads \( {p}_r^{T1} \) and \( {p}_{\theta}^{T1} \) , reduced to the bar axis (see Fig. 1). In this case, stress relations (8) and (10) remain unchanged, but displacement relations (14) become
$$ {\displaystyle \begin{array}{c}{\left.{u}_r\right|}_{r={r}_1}=\frac{F_{\theta}\left(\cos \theta -\sin \theta \right)}{2b{D}_{-1}}-\frac{F_r\left(\theta \cos \theta +\sin \theta \right)}{2b{D}_{-1}}-\frac{r_C{F}_{\theta }+M}{b{D}_0}+{K}_4\sin \theta +{K}_7\cos \theta, \\ {}{u}_{\theta }=r\left[\frac{-{F}_{\theta}\sin \theta +{F}_r\left(1-\cos \theta \right)}{b{D}_{-1}}\left(\frac{1}{r}-\frac{B_0}{B_1}\right)+\frac{r_C{F}_{\theta }+M}{b{D}_0}\left(\frac{1}{r}-\frac{B_{-1}}{B_0}\right)\theta \right]-\underset{0}{\overset{\theta }{\int }}{u}_r{\left|{}_{r={r}_1} d\theta +{u}_{\theta}\right|}_{\theta =0}.\end{array}} $$
(55)
In relations (54) and (55), the following designations for the definite integrals have been used:
$$ {\displaystyle \begin{array}{c}\begin{array}{ccc}{B}_0=\underset{r_1}{\overset{r_2}{\int }}{\mu}_{\theta}^E dr,& {B}_1=\underset{r_1}{\overset{r_2}{\int }}\left({\mu}_{\theta}^Er\right) dr,& {B}_{-1}=\underset{r_1}{\overset{r_2}{\int }}\frac{\mu_{\theta}^E}{r} dr,\end{array}\\ {}{D}_{-1}=\underset{r_1}{\overset{r_2}{\int }}\left(\frac{1}{r^2}\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr-\frac{B_0}{B_1}\frac{1}{r^2}\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr\right) dr,\\ {}{D}_0=\underset{r_1}{\overset{r_2}{\int }}\left(\frac{1}{r_1}\underset{r_1}{\overset{r}{\int }}\frac{\mu_{\theta}^E}{r} dr-\frac{B_{-1}}{B_0}\underset{r_1}{\overset{r}{\int }}{\mu}_{\theta}^E dr\right) dr.\end{array}} $$
(56)
As is seen, if the stresses of transverse shear and compression are neglected, unknown remain only three constants of integration, which simplifies the use of the solution obtained. But this can lead to significant discrepancies in determining SSS of the bar if values of the ratios \( {E}_{\theta}^{\left[k\right]}/{E}_r^{\left[k\right]} \) and \( {E}_{\theta}^{\left[k\right]}/{G}_{r\theta}^{\left[k\right]} \) of its layer materials are great.