Multi-Messenger Astrophysics and the Epistemic Reasons for Cooperative Behavior.

Cooperative phenomena in science are frequently viewed as the result of social forces and material conditions within a given social system of knowledge. In this context, scientific requirements often remain in the background, if not entirely overlooked, in discussions about what motivates cooperatio...

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Publicado en:Centaurus: Journal of the European Society for the History of Science Vol. 67; no. 1; pp. 121 - 143
Autor principal: GUZZARDI, LUCA
Formato: Artículo
Publicado: Brepols Publishers 2025
Materias:
Acceso en línea:Ver este registro en EBSCOhost
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        atl: Multi-Messenger Astrophysics and the Epistemic Reasons for Cooperative Behavior.
      aug:
        au: GUZZARDI, LUCA
        affil: Università degli Studi di Milano, Italy
      su:
        Neutrino astrophysics
        Epistemics
        Cooperative research
        Cooperativeness
        Scientific models
        Astrophysics
      sug:
        subj:
          Neutrino astrophysics
          Epistemics
          Cooperative research
          Cooperativeness
          Scientific models
          Astrophysics
      keyword:
        Data Models
        Multi-Messenger Astrophysics/Astronomy
        Neutrino Astronomy
        Scientific Collaboration
        Scientific Models
        SN 1987A
      ab: Cooperative phenomena in science are frequently viewed as the result of social forces and material conditions within a given social system of knowledge. In this context, scientific requirements often remain in the background, if not entirely overlooked, in discussions about what motivates cooperation. This paper challenges such interpretations using examples from the history of neutrino astronomy and recent multi-messenger discoveries. Revisiting the hierarchy of models proposed by Suppes (1962), it argues that the ethos of collaboration in multi-messenger astrophysics is primarily driven by epistemic constraints embedded within the models describing typical multi-messenger sources and processes. These constraints necessitate cooperation among multi-messenger astronomers, regardless of other motivations for their collaborative efforts and despite the complexities and challenges involved.
      pubtype: Academic Journal
      doctype: Article
      src: R
    language: English
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