Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights
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| Main Authors: | , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866910015647907840 |
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| author | Rah, Maria Mickaelian, Areg Dotti, Francesco Flammini Spurzem, Rainer |
| author_facet | Rah, Maria Mickaelian, Areg Dotti, Francesco Flammini Spurzem, Rainer |
| contents | We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emission properties, timing behavior, and spatial distributions, and discuss how theoretical models are required to interpret these observational trends. We focus on the magnetic field spin relation, including spin up through accretion in binaries and spin down driven by magnetic dipole radiation. Using numerical tools such as NBODY6++GPU, CMC, and COMPASS, we explore how dynamical interactions and binary evolution shape the properties of compact objects. Despite major progress, several open questions remain regarding binary interactions, magnetic field evolution, and the incorporation of pulsar physics into large scale simulations. Our analysis highlights the need for improved modeling frameworks to better understand the formation pathways and long term evolution of pulsars and MSPs. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2602_08065 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights Rah, Maria Mickaelian, Areg Dotti, Francesco Flammini Spurzem, Rainer High Energy Astrophysical Phenomena Astrophysics of Galaxies We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emission properties, timing behavior, and spatial distributions, and discuss how theoretical models are required to interpret these observational trends. We focus on the magnetic field spin relation, including spin up through accretion in binaries and spin down driven by magnetic dipole radiation. Using numerical tools such as NBODY6++GPU, CMC, and COMPASS, we explore how dynamical interactions and binary evolution shape the properties of compact objects. Despite major progress, several open questions remain regarding binary interactions, magnetic field evolution, and the incorporation of pulsar physics into large scale simulations. Our analysis highlights the need for improved modeling frameworks to better understand the formation pathways and long term evolution of pulsars and MSPs. |
| title | Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights |
| topic | High Energy Astrophysical Phenomena Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2602.08065 |