Abstract
On the basis of our theoretical speculations we propose to organize search observations of baryon structures at high redshifts (z > 5). We suggest a new observable strategy for the search of baryon structures in radiolines of simplest molecules OH and CH, which may produce the megamaser and gigamaser emission in very early epoches. The theoretical basis is the possibility of seed productions for baryon structures by a last relativistic phase transition in gas of pseudo-Gold-stone bosons at z ∼ 10-20.
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