Area covering for functions regular in an annulus
G. K. ANTONYUK
Submitted 1957-01-01 | SovietRxiv: ru-195701.05309 | Translated from Russian

Abstract Generated abstract

This paper studies covering area questions for functions regular in an annulus whose logarithmic derivative has winding number at least one around nontrivial contours. It revises an earlier notion of the “star” of the Riemann surface associated with such mappings, giving a construction by nested cuts along rays from the origin through branch and boundary contact points. The construction establishes the existence and basic simple connectivity properties of the star, and yields a sharpened area inequality relating the area of the star and the area of its transform: \((1+S/\pi)(1+s/\pi)\geq R^4\), with equality only for rotations \(f(z)=\varepsilon z\).

Full Text

MATHEMATICS

G. K. ANTONYUK

COVERING OF AREAS FOR FUNCTIONS REGULAR IN AN ANNULUS

(Presented by Academician V. I. Smirnov, 22 XI 1956)

A function \(w=f(z)\in\mathfrak M\) if in the annulus \(1<|z|<R\) \(w=f(z)\) is regular and

\[ \frac{1}{2\pi i}\int_L \frac{f'(z)}{f(z)}\,dz \geqslant 1, \]

where \(L\) is a contour not homologous to zero.

The question of covering areas for functions of the class \(\mathfrak M\) was posed by G. Ya. Khazaliya in the papers \((^{1,2})\). In paper \((^1)\) the problem of minimizing the area of the image obtained under the mapping of the annulus \(1<|z|<R\) by a function \(w=f(z)\in\mathfrak M\) is solved. In paper \((^2)\) the notion of a star of the Riemann surface onto which the annulus \(1<|z|<R\) is mapped by a function \(w=f(z)\in\mathfrak M\) is introduced, and its area \(S^*\) is estimated: \(S^*\geqslant \pi(R^2-1)\). Unfortunately, the definition of a star has shortcomings, which, in particular, were pointed out in \((^3)\); moreover, the existence of a star was not proved. We give a somewhat different definition of a star (cf. \((^{2,4})\)).

  1. Let \(\mathfrak R\) and \(\mathfrak R_{\tau,\sigma}\) be Riemann surfaces onto which, respectively, the annuli \(1<|z|<R\) and \(1+\tau<|z|<R-\sigma\), \(\tau,\sigma>0\), are mapped by the function \(w=f(z)<\mathfrak M\); let \(\Gamma_\tau,\Gamma_\sigma\) be the images of the circles \(|z|=1+\tau\) and \(|z|=R-\sigma\), obtained under this mapping. Let two arbitrary sequences of numbers \(\tau_n\to0\) and \(\sigma_n\to0\), \(n\to\infty\), be given, satisfying the conditions: \(\tau_k>\tau_{k+1}\), \(\sigma_k>\sigma_{k+1}\), \(k=1,2,\ldots\). Let an arbitrary system of rays \(L_k\), \(k=1,2,\ldots,m\), drawn from the point \(w=0\), be given.

  2. We cut the Riemann surface \(\mathfrak R_{\tau_1,\sigma_1}\) over all its sheets:

a) by the system of rays \(L_k\), \(k=1,2,\ldots,m\);

b) by the system of rays drawn from the point \(w=0\) through all branch points of \(\overline{\mathfrak R_{\tau_1,\sigma_1}}\);

c) by the system of all rays issuing from the point \(w=0\) and touching the boundary of the Riemann surface \(\mathfrak R_{\tau_1,\sigma_1}\).

The same rays cut each of the Riemann surfaces \(\mathfrak R_{\tau_2,\sigma_2}\), \(\mathfrak R_{\tau_3,\sigma_3},\ldots\) into a certain totality of parts. Let \(\omega_1,\omega_2,\ldots,\omega_s\) be the sectors formed by neighboring rays of the indicated subdivision, and let their apertures be equal, respectively, to \(\alpha_1,\alpha_2,\ldots,\alpha_s\). Among the parts of the Riemann surfaces obtained under the indicated subdivision and contained in the sector \(\omega_q\), \(q=1,2,\ldots,s\), we single out all possible sequences of them (let their number be \(k_q\)*) of the form

\[ \mathfrak R_{\tau_1,\sigma_1}^{q,j}\subset \mathfrak R_{\tau_2,\sigma_2}^{q,j}\subset \mathfrak R_{\tau_3,\sigma_3}^{q,j}\subset \ldots,\quad j=1,2,\ldots,k_q\ (k_q\geqslant 1),\quad 1\leqslant q\leqslant s, \]

where \(\mathfrak R_{\tau_k,\sigma_k}^{q,j}\) is such a part of the Riemann surface \(\mathfrak R_{\tau_k,\sigma_k}\), \(k=1,2,\ldots\), lying in the sector \(\omega_q\), that the increment of \(\arg w\) along all pieces \(\Gamma_{\tau_k},\Gamma_{\sigma_k}\) entering the boundary of \(\mathfrak R_{\tau_k,\sigma_k}^{q,j}\), when they are traversed in the positive direction, is respectively equal to \(-\alpha_q\) and \(+\alpha_q\).

  1. On the Riemann surface \(\mathfrak R_{\tau_2,\sigma_2}\), \(1\leqslant q\leqslant s\), \(1\leqslant j\leqslant k_q\), mark:

a) all branch points of \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\), whose projection onto the \(w\)-plane lies outside the projection of \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\);

* It is clear that the number \(k_q\) of sequences depends on the structure of the Riemann surface.

b) all those points of the boundary of the Riemann surface \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\) which have projection onto the \(w\)-plane outside the projection of \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\), at which the rays drawn from the point \(w=0\) touch the boundary of \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\).

From the point \(w=0\), through the marked points, draw a system of rays. Cut the Riemann surface \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\) along all its sheets in the following way: draw a cut, not passing along \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\), from each of the marked points along the corresponding ray to \(w=\infty\) or \(w=0\). Among the parts of the Riemann surface obtained under such a partition, choose the one which contains \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\); denote it by \(V_{\tau_2,\sigma_2}^{q,j}\). On the Riemann surface \(\mathfrak R_{\tau_3,\sigma_3}^{q,j}\), by means of \(V_{\tau_2,\sigma_2}^{q,j}\), mark all points of the same type as the points marked by us on \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\) by means of \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\). Add to them the points marked by us earlier on \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\). Separate from the surface \(\mathfrak R_{\tau_3,\sigma_3}^{q,j}\), by means of \(V_{\tau_2,\sigma_2}^{q,j}\), the part \(V_{\tau_3,\sigma_3}^{q,j}\) by partitioning it along the rays drawn from the point \(w=0\) through the resulting set of points, just as we separated \(V_{\tau_2,\sigma_2}^{q,j}\) from \(\mathfrak R_{\tau_2,\sigma_2}^{q,j}\) by means of \(\mathfrak R_{\tau_1,\sigma_1}^{q,j}\).

Continuing in the same way the partition of the Riemann surfaces
\(\mathfrak R_{\tau_4,\sigma_4}^{q,j}\), \(\mathfrak R_{\tau_5,\sigma_5}^{q,j}\), \(\ldots\), we obtain a sequence of their parts:

\[ V_{\tau_1,\sigma_1}^{q,j}=\mathfrak R_{\tau_1,\sigma_1}^{q,j}\subset V_{\tau_2,\sigma_2}^{q,j}\subset V_{\tau_3,\sigma_3}^{q,j}\subset\ldots . \]

In this case the parts \(V_{\tau_k,\sigma_k}^{q,j}\), \(k=1,2,\ldots\), are simply connected; every ray drawn from the point \(w=0\) through a point of \(V_{\tau_k,\sigma_k}^{q,j}\) has only one segment which is a cross-section of \(V_{\tau_k,\sigma_k}^{q,j}\); the increment of \(\arg w\) along all arcs \(\Gamma_{\tau_k}\), \(\Gamma_{\sigma_k}\) entering into the boundary of \(V_{\tau_k,\sigma_k}^{q,j}\), when they are traversed in the positive direction, is respectively equal to \(-\alpha_q\) and \(+\alpha_q\).

  1. Let \(j_q\) \((q=1,2,\ldots,s)\) be some arbitrary number among the numbers \(1,2,\ldots,k_q\). Denote by \(V_n(j_1,\ldots,j_s)\) the totality of the domains

\[ \sum_{q=1}^{s} V_{\tau_n,\sigma_n}^{q,j_q},\qquad n=1,2,\ldots . \]

The star \(\mathfrak R^*\) of the Riemann surface \(\mathfrak R\) with respect to the system \(L_k\), \(k=1,2,\ldots,m\), of rays drawn from the point \(w=0\), is the open set situated on the Riemann surface \(\mathfrak R\) and which is the limiting set for some sequence \(V_n(j_1,j_2,\ldots,j_s)\) as \(n\to\infty\) (it is clear that if at least one of the numbers \(k_1,k_2,\ldots,k_s\) is greater than one, then the star is not unique).

It is evident that the star \(\mathfrak R^*\) is simply connected and that a ray drawn from the point \(w=0\) through a point of \(\mathfrak R^*\) has only one segment, lying in \(\mathfrak R^*\), with endpoints on the boundary of \(\mathfrak R^*\).

The star defined in the indicated manner exists. Using the method of A. F. Bermant \(({}^5)\), p. 192, one can obtain a result more general than the result of G. Ya. Khazalia:

\[ \left(1+\frac{S}{\pi}\right)\left(1+\frac{s}{\pi}\right)\geq R^4, \]

where \(S\) is the area of the star, \(s\) is the area of its transform; equality is possible only for the function \(f(z)=\varepsilon z\), \(|\varepsilon|=1\).

Received
20 XI 1956

CITED LITERATURE

\({}^{1}\) G. Ya. Khazalia, DAN, 20, No. 2–3 (1938).
\({}^{2}\) G. Ya. Khazalia, Tr. Matem. inst. im. Razmadze, AN GruzSSR, 18, 245 (1951).
\({}^{3}\) Math. Rev., 14, No. 6, 549 (1953).
\({}^{4}\) A. F. Bermant, Matem. sborn., 20, 55 (1947).
\({}^{5}\) G. M. Goluzin, Geometric Theory of Functions of a Complex Variable, 1952.

Submission history

Area covering for functions regular in an annulus