重力星和 JWST 催化的星系形成再探

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astrophysics and Space Science Pub Date : 2024-07-02 DOI:10.1007/s10509-024-04334-2
Stephen L. Adler
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引用次数: 0

摘要

我们曾提出,星系的形成是由来自泄漏的无视界天体物理黑洞(很可能是引力星)的内流粒子和外流粒子的碰撞催化的,并在此基础上给出了一个盘状星系尺度长度模型。在本文中,我们修改了最初的尺度长度公式,加入了碰撞导致恒星形成成核的活化概率\(P\)。修改后的公式从早期宇宙的JWST数据推断到晚期数据的误差在5倍以内,并表明星系的尺寸应该随着观测到的红移z的增加而系统地变小。我们还表明,粒子通过引力星的循环可以通过 "热泵 "制冷效应降低周围气体的温度。这可以通过增强引力星附近恒星的形成来触发星系的形成。
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Galaxy formation catalyzed by gravastars and the JWST, revisited

We have proposed that galaxy formation is catalyzed by the collision of infalling and outstreaming particles from leaky, horizonless astrophysical black holes, most likely gravastars, and based on this gave a model for the disk galaxy scale length. In this paper we modify our original scale length formula by including an activation probability \(P\) for a collision to lead to nucleation of star formation. The revised formula extrapolates from early universe JWST data to late time data to within a factor of five, and suggests that galaxy dimensions should systematically get smaller as the observed redshift z increases. We also show that particles recycling through gravastars can lead to a reduction in the temperature of the surrounding gas, through a “heat pump” refrigeration effect. This can trigger galaxy formation through enhanced star formation in the vicinity of the gravastar.

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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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