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<title>Mathematical Sciences</title>
<link>http://hdl.handle.net/123456789/1</link>
<description/>
<item>
<title>Verovatnosni računi sekvenata i klasifikacija neklasičnih logika zasnovana na entropiji</title>
<link>http://hdl.handle.net/123456789/5834</link>
<description>Verovatnosni računi sekvenata i klasifikacija neklasičnih logika zasnovana na entropiji

Boričić, Marija

After a brief introductory survey, this work is divided into two parts. The first&#13;
part deals with presence of probability in logic (v. [16], [17], [18], [19], [22], [23] and&#13;
[24]), and the second one is devoted to the application of entropy in classification of&#13;
many–valued logics (v. [14], [15], [20], [21] and [25]).&#13;
The basic idea, dominant in the first part of the work, is to enrich the Gentzen’s&#13;
sequent calculus LK for propositional classical logic by a kind of probability operator&#13;
defined over the sequents ¡ ` ¢ in order to express the fact that ”the truthfulness&#13;
probability of ¡ ` ¢ belongs to the interval [a; b] µ [0; 1]”. We introduce the&#13;
following four systems: LKprob, LKprob("), NKprob and LKfuzz. The basic&#13;
form of sequents in LKprob is ¡ `b&#13;
a ¢ with the above given intended meaning. The&#13;
system LKprob(") is focused on the Suppes’ forms ¡ `n ¢ enabling to formalize&#13;
the sentence ”the truthfulness probability of ¡ ` ¢ belongs to the interval [1 ¡&#13;
n"; 1] µ [0; 1]”, for some n 2 N. The system NKprob presents a natural deduction&#13;
counterpart of the sequent calculus LKprob. The models founded on Carnap–&#13;
Popper–Leblance probability semantics are defined for each of these calculi and&#13;
accompanied by the corresponding soundness and completeness results. Finally, the&#13;
calculus LKfuzz is introduced with a more general form of the sequents ¡ `x ¢,&#13;
where x is an element of a finite lattice, with the aim to describe a fuzzification&#13;
of LK. The meaning of ¡ `x ¢ is that ”x is the fuzziness measure of ¡ ` ¢”.&#13;
Models for LKfuzz are given with soundness and completeness results, and a proof–&#13;
theoretical treatment of LKfuzz includes the cut–elimination theorem.&#13;
The second part of the work explores the fact that each logical system associated&#13;
with the partition induced by the corresponding Lindenbaum–Tarski algebra makes&#13;
it possible to define its entropy. We define the entropy of a logical system based on&#13;
geometric distribution of measures over matching partition of set of formulae. This&#13;
iv&#13;
definition enables the classification of many–valued propositional logics according to&#13;
their entropies. Asymptotic entropy approximations for some infinite–valued logics&#13;
are proposed as well. The considered examples include Lukasiewicz’s, Kleene’s and&#13;
Priest’s three–valued logics, Belnap’s four–valued logic, G¨odel’s and McKay’s m–&#13;
valued logics, and Heyting’s and Dummett’s infinite–valued logics.

</description>
<pubDate>Fri, 01 Jan 2016 00:00:00 GMT</pubDate>
</item>
<item>
<title>Ostatak određenih tipova Gausovih kvadraturnih formula sa specijalnim klasama težinskih funkcija</title>
<link>http://hdl.handle.net/123456789/5833</link>
<description>Ostatak određenih tipova Gausovih kvadraturnih formula sa specijalnim klasama težinskih funkcija

Mihić, Ljubica

Mathematical modeling of many phenomena which occur in the&#13;
natural, technical sciences, economy requires signi cant knowledge of&#13;
the theory of numerical integration. In the situations where the integral&#13;
cannot be determined analytically, it is necessary to construct the for-&#13;
mula which approximates its value with acceptable error. Besides the&#13;
traditional formulae, the tendencies in the development of this area refer&#13;
to increment of algebraic degree of precision of the quadrature formula&#13;
and its error estimation.&#13;
The subject of this dissertation is Gaussian quadrature formula with&#13;
increased number of nodes which may have double multiplicity (sections&#13;
2 and 4) or arbitrary multiplicity (section 3). When we consider the&#13;
addition of one node, one of the integration interval ends, the&#13;
corresponding quadrature formula is called Gauss-Radau, and in the case&#13;
of adding two new nodes, the appropriate formula is of Gauss-Lobatto&#13;
type. Beside those formulae, in this dissertation we consider the&#13;
Kronrod's extension of Gauss-Tur an quadrature formula, which includes&#13;
the derivatives of the function at nodes. Here, the main aim is to deter-&#13;
mine efficient error bounds of these formulae with respect to the&#13;
different types of Chebyshev weight functions and Gori-Micchelli weight&#13;
function which, in one special case, represents the generalization of the&#13;
 rst Chebyshev weight function.&#13;
Introductory theorems and well-known statements that are used in&#13;
the rest of the thesis are presented in the  rst section. We described basic&#13;
properties of orthogonal polynomials participating in the construction&#13;
of Gaussian quadrature formula. Furthermore, the different types of&#13;
remainder terms of quadrature formula are de ned, whereby in the&#13;
following sections we analyze the integral representation of the remainder&#13;
term. The recent results relating to the increasing number of the nodes of&#13;
arbitrary multiplicity are exposed. The remaining three sections contain&#13;
the chapters with original results.&#13;
The second section is devoted to the estimation of the error of Gauss-&#13;
Lobatto quadrature formulae with a double nodes at the endpoints. Af-&#13;
ter detailed analysis of the kernel of the remainder term (see subsection&#13;
2.2.1), we proved the Theorems stating the behavior of the maximum&#13;
modulus of the kernel. We computed  xed values mentioned in the The-&#13;
orems and established the real errors and the error bounds of quadrature&#13;
formula.&#13;
In third section we examine the Kronrod's extension of Gauss-&#13;
Tur an quadrature formulae with respect to the special kind of Gori-&#13;
Micchelli weight function. This extension, beside the nodes of Gauss-&#13;
Tur an quadrature formula, also contains the zeros of Chebyshev polyno-&#13;
mial of the second kind. In those new nodes, we consider just the values&#13;
of the function (not the values of its derivatives). Previously mentioned&#13;
Kronrod's extension is actually Chakalov-Popoviciu quadrature formu-&#13;
la, so, by applying the methods for those formulae, we computed the&#13;
coefficients and the error of Kronrod's formula.&#13;
Gautschi-Li hypotheses are proven in the fourth section. Those&#13;
hypotheses concern the Gauss-Radau quadrature formulae with respect&#13;
to the Chebyshev weight functions of the second and the third kind.&#13;
Subsection 4.4 consists of numerical examples and the tables with&#13;
efficient error bounds.

</description>
<pubDate>Sun, 01 Jan 2017 00:00:00 GMT</pubDate>
</item>
<item>
<title>OPTIČKA DETEKCIJA OSTATAKA SUPERNOVIH I UTICAJ NJIHOVE EMISIJE U LINIJI Hα NA ODREDIVANJE STOPE FORMIRANJA ZVEZDA</title>
<link>http://hdl.handle.net/123456789/5832</link>
<description>OPTIČKA DETEKCIJA OSTATAKA SUPERNOVIH I UTICAJ NJIHOVE EMISIJE U LINIJI Hα NA ODREDIVANJE STOPE FORMIRANJA ZVEZDA

Vučetić, Milica

In this dissertation we discuss in uence of H emission from supernova remnants&#13;
(SNRs) on H derived star formation rates (SFRs). We present the detection of 16&#13;
optical SNR candidates in a part of nearby spiral galaxy IC342, and two more poten-&#13;
tial SNRs in NGC 185 galaxy. The candidates were detected by applying [S ii]/H&#13;
ratio criterion on observations made with the 2 m telescope at Rozhen National&#13;
Astronomical Observatory in Bulgaria. Also, in this dissertation we present the&#13;
most up-to-date list of nearby galaxies with optically detected SNRs. When deri-&#13;
ving H star formation rates, assumption is that the radiation is coming from the&#13;
ionized gas surrounding hot and young stars { H ii regions. In this case, emission&#13;
from SNRs contaminates H ux used to derive SFR. We found that the contribu-&#13;
tion of SNRs' ux to the total H ux, for 18 galaxies in our sample of galaxies&#13;
with optical SNRs, is 5   5%. Due to the observational selection effects, the SNR&#13;
contamination of SFRs derived herein represents only a lower limit. M83 is the&#13;
galaxy with the most detected optical SNRs and in this galaxy SNRs account for&#13;
9 per cent of the total H emission. We expect that fraction similar to this would&#13;
be close to the real contribution of SNR emission to the total H emission in spiral&#13;
galaxies.&#13;
Using two dwarf galaxies as an example, Holmberg IX and NGC 185, we show&#13;
that the contamination of H ux by SNRs, or other sources, can be much larger,&#13;
up to ten times higher than total H ux coming from H ii regions of the observed&#13;
galaxy.

</description>
<pubDate>Sun, 01 Jan 2017 00:00:00 GMT</pubDate>
</item>
<item>
<title>POLINOMIJALNA ENTROPIJA INDUKAOVANIH DINAMIČKIH SISTEMA NA HIPERPROSTORIMA</title>
<link>http://hdl.handle.net/123456789/5828</link>
<description>POLINOMIJALNA ENTROPIJA INDUKAOVANIH DINAMIČKIH SISTEMA NA HIPERPROSTORIMA

Đorić, Maša

In this thesis, we applied a method for computing the polynomial entropy of&#13;
dynamical systems with a finite non-wandering set to certain hyperspaces of the interval and&#13;
the circle. We subsequently generalized these results to the case where the non-wandering&#13;
set is not finite. We proved that the polynomial entropy of the induced map C(f ) is equal&#13;
to 2, that of Fn(f ) is equal to n, and that of 2f is infinite, when f is a homeomorphism of&#13;
the interval or the circle. Furthermore, we generalized these results for the n-fold symmetric&#13;
product of the interval and the circle to an arbitrary compact metric space X and extended&#13;
them to the suspension of the space Fn(X). In addition to the results on hyperspaces, we&#13;
presented results concerning polynomial entropy on certain one-dimensional continua, such&#13;
as local dendrites and regular curves. We also constructed a family of pointwise periodic&#13;
homeomorphisms on a continuum whose polynomial entropy attains every value in [0, +∞].

</description>
<pubDate>Tue, 01 Sep 2026 00:00:00 GMT</pubDate>
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