A proposal for a fast infrared bursts detector

IF 17.7 1区 化学 Q1 CHEMISTRY, MULTIDISCIPLINARY Accounts of Chemical Research Pub Date : 2024-05-01 DOI:10.1088/1748-0221/19/05/p05027
A. Drago, S. Bini, M. Cestelli Guidi, A. Marcelli, Valerio Bocci, E. Pace
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Abstract

The gravitational wave GW170817 from a binary neutron star merger and the simultaneous electromagnetic detection of the GRB170717A by Fermi Gamma-Ray Space Telescope, opened a new era in the multi-messenger astronomy. Furthermore, the GRBs (Gamma-Ray Bursts) and the mysterious FRBs (Fast Radio Bursts) have sparked interest in the development of new detectors and telescopes dedicated to the time-domain astronomy across the electromagnetic spectrum. Time-domain astronomy aims to acquire fast astronomical bursts in temporal range between a few seconds down to 1 ns. Fast InfraRed Bursts (FIRB's) have been relatively understudied, often due to the lack of appropriate tools for observation and analysis. In this scientific scenario, the present contribution proposes a new detection system for ground-based reflecting telescopes working in the mid-infrared (mid-IR) range to search for astronomical FIRB's. Experience developed in the diagnostics for lepton circular accelerators can be used to design temporal devices for astronomy. Longitudinal diagnostic instruments acquire bunch-by-bunch particle shifts in the direction of flight, that is equivalent to temporal. Transverse device integrates the beam signal in the horizontal and vertical coordinates, as standard telescopes. The proposed instrument aims to work in temporal mode. Feasibility study tests have been carried out at SINBAD, the infrared beam line of DAFNE, the e+e- collider of INFN. SINBAD releases pulsed infrared synchrotron light with 2.7 ns separation. The front-end detector system has been evaluated to detect temporal fast infrared signals with 2–12 μm wavelengths and 1 ns rise times. The present contribute aims to be a step toward a feasibility study report.
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关于快速红外猝发探测器的建议
双中子星合并产生的引力波 GW170817 和费米伽马射线太空望远镜同时探测到的电磁波 GRB170717A 开启了多信使天文学的新纪元。此外,GRB(伽马射线暴)和神秘的 FRB(快速射电暴)也引发了人们对开发新的探测器和望远镜的兴趣,这些探测器和望远镜专门用于整个电磁频谱的时域天文学。时域天文学旨在获取时间范围在几秒到 1 ns 之间的快速天文爆发。对快速红外脉冲串(FIRB)的研究相对较少,这往往是因为缺乏适当的观测和分析工具。在这一科学背景下,本论文提出了一种新的探测系统,用于中红外(mid-IR)范围内的地基反射望远镜,以搜寻天文中的快速红外暴。在轻子环形加速器诊断方面积累的经验可用于设计天文学的时间装置。纵向诊断仪器获取粒子束在飞行方向上的逐束偏移,这相当于时间诊断。横向设备在水平和垂直坐标上整合光束信号,就像标准望远镜一样。拟议的仪器旨在以时间模式工作。已经在 SINBAD、DAFNE 的红外光束线和 INFN 的 e+e- 对撞机上进行了可行性研究测试。SINBAD 释放的脉冲红外同步加速器光的间隔为 2.7 ns。对前端探测器系统进行了评估,以探测波长为 2-12 μm、上升时间为 1 ns 的时间快速红外信号。本报告旨在向可行性研究报告迈出一步。
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来源期刊
Accounts of Chemical Research
Accounts of Chemical Research 化学-化学综合
CiteScore
31.40
自引率
1.10%
发文量
312
审稿时长
2 months
期刊介绍: Accounts of Chemical Research presents short, concise and critical articles offering easy-to-read overviews of basic research and applications in all areas of chemistry and biochemistry. These short reviews focus on research from the author’s own laboratory and are designed to teach the reader about a research project. In addition, Accounts of Chemical Research publishes commentaries that give an informed opinion on a current research problem. Special Issues online are devoted to a single topic of unusual activity and significance. Accounts of Chemical Research replaces the traditional article abstract with an article "Conspectus." These entries synopsize the research affording the reader a closer look at the content and significance of an article. Through this provision of a more detailed description of the article contents, the Conspectus enhances the article's discoverability by search engines and the exposure for the research.
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