观测到的快速射电暴种群趋势和光密度分布的双模态

IF 1.9 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY
Pramana Pub Date : 2025-01-30 DOI:10.1007/s12043-024-02881-5
Nidhi Saini, Gupta Patrick Das
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引用次数: 0

摘要

快速射电暴(frb)是源自河外的无线电瞬变现象,持续时间从几分之一毫秒到数百毫秒不等。它们的实际物理性质尚未确定,仍然是一个积极研究的课题。在本文中,我们考虑了非CHIME和CHIME源,并对可用的FRB数据进行了各种分析。由于CHIME第一个目录只提供了快速射电暴通量密度和通量的下限,我们设计了一种新的方法,利用已编目的通量密度下限\(S_{\nu _O}\)与单个快速射电暴事件通量\(F_{\nu _O}\)的比值来构建几个参数\(Xi, i=1,2,\ldots ,7\)但\( i \ne 5\),以研究CHIME快速射电暴种群中潜在趋势的存在。对于非chime快速射电暴事件,也可以使用测量的通量密度\(S_{\nu _O}\)与通量\(F_{\nu _O}\)之比来计算这些参数。其中一个定义的参数(X7)涉及实际的亮度温度和能量密度,而不是相应的边界,尽管人们忽略了FRB发射区域的实际大小。我们的第一个强有力的结论是,单个非chime快速射电暴事件可根据其峰值亮度密度分为两大类。这已经明确地证明了在两个不同的频率- 300和450 MHz计算的峰值亮度密度。我们的第二个可靠结果是,CHIME和非CHIME FRB种群中涉及通量密度与通量之比的参数Xis几乎是相同的,这证明我们使用这些参数来利用\(S_{\nu _O}/ F_{\nu _O}\)和其他测量量是正确的。这种普遍性也体现在CHIME和非CHIME快速射电暴种群计算参数Xis分布的基本模式中,从而表明即使是CHIME探测到的快速射电暴事件也存在两类。假设快速射电暴是由导致光柱半径突变的磁星故障引起的,我们考虑了一个简单的物理模型来解决基于快速射电暴亮度密度的两类问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Observed trends in FRB population and bi-modality in the luminosity density distribution

Observed trends in FRB population and bi-modality in the luminosity density distribution

Fast radio bursts (FRBs) are radio-transients of extragalactic origin lasting from fractions of a millisecond to hundreds of milliseconds. Their actual physical nature is yet to be ascertained and is still a topic of active research. In this paper, we have considered both non-CHIME and CHIME sources, and have subjected the available FRB data to various analyses. Since CHIME first catalogue provides only the lower bounds to the FRB flux density and fluence, we have devised a novel approach that utilises the ratio of the catalogued lower limits of the flux density \(S_{\nu _O}\) to the fluence \(F_{\nu _O}\) of individual FRB events to construct several parameters \(Xi, i=1,2,\ldots ,7\) but \( i \ne 5\) to investigate the presence of underlying trends in the CHIME FRB population. These parameters are also computed for the non-CHIME FRB events using the ratio of the measured flux density \(S_{\nu _O}\) to the fluence \(F_{\nu _O}\). One of these defined parameters (X7) involve the actual brightness temperature as well as energy density instead of the corresponding bounds, despite one’s ignorance of thess actual size of the FRB emission region. Our first robust conclusion is that the individual non-CHIME FRB events fall under two broad categories based on their peak luminosity densities. This has been explicitly demonstrated for peak luminosity densities calculated at two distinct frequencies – 300 and 450 MHz. Our second robust result is that the parameters Xis involving the ratio of the flux density to the fluence are almost the same for both CHIME and non-CHIME FRB populations, vindicating our use of these parameters that make use of \(S_{\nu _O}/ F_{\nu _O}\) and other measured quantities. This universality is also seen in the underlying patterns exhibited by the distributions of the computed parameters Xis for both CHIME and non-CHIME FRB population, suggesting thereby the existence of two categories even for the FRB events detected by CHIME. Assuming that FRBs are caused by magnetar glitches that lead to an abrupt change in the light cylinder radius, we have considered a simple physical model to address the issue of two categories based on the FRB luminosity density.

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来源期刊
Pramana
Pramana 物理-物理:综合
CiteScore
3.60
自引率
7.10%
发文量
206
审稿时长
3 months
期刊介绍: Pramana - Journal of Physics is a monthly research journal in English published by the Indian Academy of Sciences in collaboration with Indian National Science Academy and Indian Physics Association. The journal publishes refereed papers covering current research in Physics, both original contributions - research papers, brief reports or rapid communications - and invited reviews. Pramana also publishes special issues devoted to advances in specific areas of Physics and proceedings of select high quality conferences.
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