{"title":"用GRAMS实验搜索反氦-3","authors":"J. Zeng","doi":"10.22323/1.444.1407","DOIUrl":null,"url":null,"abstract":"Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation experiment using a Liquid Argon Time Projection Chamber (LArTPC) to detect gamma rays and antiparticles. Especially for antiparticle detection, GRAMS could reach high sensitivity within the low energy region (< 0.5GeV ) using a cost-effective LArTPC design. GRAMS is projected to be able to make background-free dark matter measurements from antimatter detection in the energy range of 0.1-0.5 GeV/n. In this poster, I will introduce the GRAMS detection concept and particle identification techniques. With the GRAMS instrument, we could detect antiprotons, antideuterons and potentially antihe-lium nuclei. I will introduce the method of separating antihelium from the antiproton background. Based on this method, I will talk about the flux limit that GRAMS can reach for antihelium-3. This method will provide an opportunity to test a variety of dark matter models.","PeriodicalId":448458,"journal":{"name":"Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)","volume":"38 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-08-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"AntiHelium-3 Search with the GRAMS Experiment\",\"authors\":\"J. Zeng\",\"doi\":\"10.22323/1.444.1407\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation experiment using a Liquid Argon Time Projection Chamber (LArTPC) to detect gamma rays and antiparticles. Especially for antiparticle detection, GRAMS could reach high sensitivity within the low energy region (< 0.5GeV ) using a cost-effective LArTPC design. GRAMS is projected to be able to make background-free dark matter measurements from antimatter detection in the energy range of 0.1-0.5 GeV/n. In this poster, I will introduce the GRAMS detection concept and particle identification techniques. With the GRAMS instrument, we could detect antiprotons, antideuterons and potentially antihe-lium nuclei. I will introduce the method of separating antihelium from the antiproton background. Based on this method, I will talk about the flux limit that GRAMS can reach for antihelium-3. This method will provide an opportunity to test a variety of dark matter models.\",\"PeriodicalId\":448458,\"journal\":{\"name\":\"Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)\",\"volume\":\"38 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-08-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22323/1.444.1407\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22323/1.444.1407","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation experiment using a Liquid Argon Time Projection Chamber (LArTPC) to detect gamma rays and antiparticles. Especially for antiparticle detection, GRAMS could reach high sensitivity within the low energy region (< 0.5GeV ) using a cost-effective LArTPC design. GRAMS is projected to be able to make background-free dark matter measurements from antimatter detection in the energy range of 0.1-0.5 GeV/n. In this poster, I will introduce the GRAMS detection concept and particle identification techniques. With the GRAMS instrument, we could detect antiprotons, antideuterons and potentially antihe-lium nuclei. I will introduce the method of separating antihelium from the antiproton background. Based on this method, I will talk about the flux limit that GRAMS can reach for antihelium-3. This method will provide an opportunity to test a variety of dark matter models.