Christina Schwemmbauer, Yonit Hochberg, K. Isleif, F. Januschek, Benjamin Lehmann, A. Lindner, Manuel Meyer, Gulden Othman, José Alejandro Rubiera Gimeno
{"title":"Simulations for direct dark matter searches using ALPS II's TES detection system","authors":"Christina Schwemmbauer, Yonit Hochberg, K. Isleif, F. Januschek, Benjamin Lehmann, A. Lindner, Manuel Meyer, Gulden Othman, José Alejandro Rubiera Gimeno","doi":"10.22323/1.454.0055","DOIUrl":"https://doi.org/10.22323/1.454.0055","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140747112","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Plasmonic resonant detection of WIMP","authors":"Carlo Alfisi, Hugo Terças","doi":"10.22323/1.454.0057","DOIUrl":"https://doi.org/10.22323/1.454.0057","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140746706","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Status of the VMB@CERN experiment","authors":"Stepan Kunc","doi":"10.22323/1.454.0032","DOIUrl":"https://doi.org/10.22323/1.454.0032","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140754046","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"In search of new particles with PADME","authors":"Radoslav Simeonov","doi":"10.22323/1.454.0043","DOIUrl":"https://doi.org/10.22323/1.454.0043","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140378976","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
The search for the existence of solar axions has been and continues to be brought forward using so-called helioscopes. In a helioscope, solar axions can travel in an evacuated volume in presence of a strong magnetic field. Along this path, axions have the possibility to convert to photons. Detecting such photons, expected to be in the keV range, will be the indication of the existence of solar axions. X-ray detectors with low background, high efficiency and high energy resolution are therefore an important component of such experiments. Metallic Magnetic Calorimeters (MMCs) are detectors operated at mK temperature which offer an energy resolution better than 10 eV full width at half maximum (FWHM) and a detection efficiency close to 100% over the energy range of interest for solar axion, including a spectral line around 14 keV generated in axion-nucleon interaction in the Sun. In addition, a very low energy threshold can be achieved, limited by the necessary window against infrared radiation. These detectors are therefore one of the technologies considered for the fourth generation helioscope IAXO. The present status of MMC optimization for IAXO will be discussed along with the importance for both the axion discovery phase and even more for the study of axion properties after discovery, thanks to the unique performance of these detectors.
人们一直在利用所谓的日光镜寻找太阳轴子的存在。在日光镜中，太阳轴子可以在强磁场的作用下在一个抽空的空间中传播。沿着这条路径，轴子有可能转换成光子。探测到这种光子（预计在 keV 范围内）将表明太阳轴子的存在。因此，具有低背景、高效率和高能量分辨率的 X 射线探测器是此类实验的重要组成部分。金属磁性量热计（MMC）是在 mK 温度下工作的探测器，其能量分辨率优于 10 eV 的半最大全宽（FWHM），在太阳轴子感兴趣的能量范围内探测效率接近 100%，包括太阳中轴子-核子相互作用产生的 14 keV 左右的光谱线。此外，受限于必要的红外辐射窗口，还可以实现非常低的能量阈值。因此，这些探测器是第四代日像仪 IAXO 考虑采用的技术之一。将讨论为 IAXO 优化 MMC 的现状，以及这些探测器的独特性能对轴心发现阶段的重要性，甚至对发现后轴心特性研究的重要性。
{"title":"High energy resolution x-ray detectors for IAXO: advantages in pre- and post-discovery phases","authors":"Loredana Gastaldo, Daniel Hengstler, Daniel Unger","doi":"10.22323/1.454.0038","DOIUrl":"https://doi.org/10.22323/1.454.0038","url":null,"abstract":"The search for the existence of solar axions has been and continues to be brought forward using so-called helioscopes. In a helioscope, solar axions can travel in an evacuated volume in presence of a strong magnetic field. Along this path, axions have the possibility to convert to photons. Detecting such photons, expected to be in the keV range, will be the indication of the existence of solar axions. X-ray detectors with low background, high efficiency and high energy resolution are therefore an important component of such experiments. Metallic Magnetic Calorimeters (MMCs) are detectors operated at mK temperature which offer an energy resolution better than 10 eV full width at half maximum (FWHM) and a detection efficiency close to 100% over the energy range of interest for solar axion, including a spectral line around 14 keV generated in axion-nucleon interaction in the Sun. In addition, a very low energy threshold can be achieved, limited by the necessary window against infrared radiation. These detectors are therefore one of the technologies considered for the fourth generation helioscope IAXO. The present status of MMC optimization for IAXO will be discussed along with the importance for both the axion discovery phase and even more for the study of axion properties after discovery, thanks to the unique performance of these detectors.","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140386210","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"CAST and more than CAST; A Dark Sector Probe for 20+ Years","authors":"Serkant Ali Cetin","doi":"10.22323/1.454.0030","DOIUrl":"https://doi.org/10.22323/1.454.0030","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140224469","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Radiation from Axion Strings with Adaptive Mesh Refinement: Periodic and Burst Signals","authors":"Amelia Drew, Tomasz Kinowski, P. Shellard","doi":"10.22323/1.454.0019","DOIUrl":"https://doi.org/10.22323/1.454.0019","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140224178","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Probing the Dark Sector with NA64 and POKER at CERN SPS","authors":"Luca Marsicano","doi":"10.22323/1.454.0036","DOIUrl":"https://doi.org/10.22323/1.454.0036","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140225938","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Using gravitational waves to detect axion miniclusters","authors":"Juan Urrutia","doi":"10.22323/1.454.0046","DOIUrl":"https://doi.org/10.22323/1.454.0046","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140233897","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Axion-like particle searches at the LHC","authors":"Michele Gallinaro","doi":"10.22323/1.454.0034","DOIUrl":"https://doi.org/10.22323/1.454.0034","url":null,"abstract":"","PeriodicalId":516989,"journal":{"name":"Proceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-03-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140256041","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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