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<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Dual-step optimization for binary sequences with high merit factors</dc:title><dc:creator>Pšeničnik,	Blaž	(Avtor)
	</dc:creator><dc:creator>Mlinarič,	Rene	(Avtor)
	</dc:creator><dc:creator>Brest,	Janez	(Avtor)
	</dc:creator><dc:creator>Bošković,	Borko	(Avtor)
	</dc:creator><dc:subject>binary sequences</dc:subject><dc:subject>Golay's merit factor</dc:subject><dc:subject>autocorrelation</dc:subject><dc:subject>algorithms</dc:subject><dc:description>The problem of finding aperiodic low auto-correlation binary sequences (LABS) presents a significant computational challenge, particularly as the sequence length increases. Such sequences have important applications in communication engineering, physics, chemistry, and cryptography. This paper introduces a dual-step algorithm for long binary sequences with high merit factors. The first step employs a parallel algorithm utilizing skew-symmetry and restriction classes to generate sequence candidates with merit factors above a predefined threshold. The second step uses a priority queue algorithm to refine these candidates further, searching the entire search space unrestrictedly. By combining GPU-based parallel computing and dual-step optimization, our approach has successfully identified best-known binary sequences for all lengths ranging from 450 to 527, with the exception of length 518, where the previous best-known merit factor value was matched with a different sequence. This hybrid method significantly outperforms traditional exhaustive and stochastic search methods, offering an efficient solution for finding long sequences with good merit factors.</dc:description><dc:publisher>Elsevier Inc.</dc:publisher><dc:date>2025</dc:date><dc:date>2025-05-30 11:16:02</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>93000</dc:identifier><dc:identifier>UDK: 004</dc:identifier><dc:identifier>COBISS_ID: 236425219</dc:identifier><dc:identifier>DOI: 10.1016/j.dsp.2025.105316</dc:identifier><dc:identifier>ISSN pri članku: 1095-4333</dc:identifier><dc:language>sl</dc:language><dc:rights>© 2025 The Author(s)</dc:rights></metadata>
