Summary
After reviewing some statistical models of multiple production, a cluster radiative emission picture in configuration space is proposed and, with the aid of an extension of the Gottfried model, the rapidity and mass distributions of clusters are determined. They agree with the independent cluster production model of Pokorski and Van Hove. Some connections with the thermodynamical model and some problems about the mass spectra are discussed.
Riassunto
Dopo una rassegna di alcuni modelli statistici di produzione multipla, si propone uno schema di emissione radiativa degli ammassi nello spazio delle configurazioni e, usando un’estensione del modello di Gottfried, si calcolano le distribuzioni in rapidità e in massa degli ammassi. Esse concordano con il modello di produzione indipendente degli ammassi di Pokorski-Van Hove. Si discutono poi alcune connessioni con il modello termodinamico e alcuni problemi sugli spettri di massa.
Реэюме
После аналиэа некоторых статистических моделей множественного рождения предлагается картина радиационной змиссии кластеров в конфигурационном пространстве. Испольэуя обобшение модели Готфрида, определяются расре-деления скоростей и масс кластеров. Полученные реэультаты согласуются с моделью рождения неэависимых кластеров Покорского-Ван Хова. Обсуждаются свяэь с термодинамической моделью и некоторые проблемы массовых спектров.
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Lusanna, L. Cluster radiative emission and statistical models. Nuov Cim A 24, 309–323 (1974). https://doi.org/10.1007/BF02821998
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DOI: https://doi.org/10.1007/BF02821998