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101.
102.
Shmuel Friedland 《Linear and Multilinear Algebra》1978,6(2):123-143
It Is shown here that a permanent of n× ndoubly stochastic matrix is not less than 1/ n!. The proof of this inequality follows from the study of a generalized van der Waerden problem on the set of doubly stochastic matrices. 相似文献
103.
Let 6x6 be a norm on Cn. For A?Mn(C) denote by 6A6 the induced norm of A, by ?(A) the spectral radius of A. It is proved here that if infp6PAP?16 = ?(A), then 6x6 is a transform absolute norm. 相似文献
104.
Archive for Rational Mechanics and Analysis - 相似文献
105.
Jean François Mertens Shmuel Zamir 《Journal of Mathematical Analysis and Applications》1977,60(2):550-558
Given P and Q convex compact sets in RkandRs, respectively, and u a continuous real valued function on P × Q, we consider the following pair of dual problems: Problem I—Minimize ? so that ?: . Problem II—Maximize g so that g: P × Q → R and g ? Vexq × Cavpmin(u, g). Here Cavp is the operation of concavification of a function with respect to the variable p?P (for each fixed q?Q). Similarly, Vexq is the operation of convexification with respect to q?Q. Maximum and minimum are taken here in the partial ordering of pointwise comparison: . It is proved here that both problems have the same solution which is also the unique simultaneous solution of the following pair of functional equations: (i) . (ii) . The problem arises in game theory, but the proof here is purely analytical and makes no use of game-theoretical concepts. 相似文献
106.
107.
Black hole formation is an inevitable consequence of relativistic core collapse following the gravothermal catastrophe in self-interacting dark matter (SIDM) halos. Very massive SIDM halos form supermassive black holes (SMBHs) > or about 10(6)M(middle dot in circle) directly. Smaller halos believed to form by redshift z = 5 produce seed black holes of (10(2)-10(3))M(middle dot in circle) which can merge and/or accrete to reach the observational SMBH range. This scenario for SMBH formation requires no baryons, no prior star formation, and no other black hole seed mechanism. 相似文献
108.
We show that direct dark-matter detection experiments can distinguish between pointlike and nonpointlike dark-matter candidates. The shape of the nuclear recoil-energy spectrum from pointlike dark-matter particles, e.g., neutralinos, is determined by the velocity distribution of dark matter in the galactic halo and by nuclear form factors. Typical cross sections of nonpointlike dark matter, for example, Q-balls, have a new form factor, which decreases rapidly with the recoil energy. A signal from nonpointlike dark matter is expected to peak near the experimental threshold and to fall off rapidly at higher energies. 相似文献
109.
k -colorable for some fixed . Our main result is that it is NP-hard to find a 4-coloring of a 3-chromatic graph. As an immediate corollary we obtain that
it is NP-hard to color a k-chromatic graph with at most colors. We also give simple proofs of two results of Lund and Yannakakis [20]. The first result shows that it is NP-hard
to approximate the chromatic number to within for some fixed ε > 0. We point here that this hardness result applies only to graphs with large chromatic numbers. The second
result shows that for any positive constant h, there exists an integer , such that it is NP-hard to decide whether a given graph G is -chromatic or any coloring of G requires colors.
Received April 11, 1997/Revised June 10, 1999 相似文献
110.
The prolongation of lifetimes for an excited atom due to the presence of nearby atoms in the ground state is shown to follow simply from unitarity of the time evolution. We also discuss possible approaches to the detection and the overcoming of various technical obstacles. 相似文献