Unavoidable stars of an n-set
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A hypergraph \( H\) consists of a vertex set \( V\) together with a family \( E\) of subsets of \( V\), which are called the edges of \( H\). A \( r\)-uniform hypergraph, or \( r\)-graph, for short, is a hypergraph whose edge set consists of \( r\)-subsets of \( V\). A graph is just a special case of an \( r\)-graph with \( r=2\).
Let us call a family \( {\mathcal S } = (S_1, S_2, \ldots, S_r)\) of \( r\)-graphs \( S_i\), a \( t\)-star with center \( A\), if for all \( i <j\), \( S_i \cap S_j = A \) (possibly empty). Stars were introduced by Erdös and Rado [2] in 1960 under the name strong delta systems, where they proved that every large \( r\)-graph contains a \( t\)-star.
A problem on unavoidable stars of an \(n\)-set (proposed by Erdös and Szemerédi [3])
Determine the least integer \(m\), denoted by \(f^*(n,k)\), such that for any family \(\mathcal{A}\) of subsets of an \(n\)-set with \(|{\mathcal{A}}| > f^*(n,k)\), \(\mathcal{A}\) must contain a \(k\)-star.Erdös and Szemerédi [3] showed that
Recently, Deuber, Erdös, Gunderson, Kostochka and Meyer [1] proved that for a fixed \( c\),