{"title":"μTRISTANμ+μ+对撞机对电弱相互作用粒子的间接探测","authors":"Risshin Okabe, Satoshi Shirai","doi":"10.1103/physrevd.110.035002","DOIUrl":null,"url":null,"abstract":"A novel collider, called <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>μ</mi><mi>TRISTAN</mi></math>, was recently proposed, offering the capability to achieve high-energy collisions of antimuons. This high-energy collider presents an exceptional opportunity for the discovery of electroweak-interacting massive particles (EWIMPs), which are predicted by various new physics models. In a lepton collider like <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>μ</mi><mi>TRISTAN</mi></math>, the potential for discovering EWIMPs extends beyond their direct production. Quantum corrections arising from EWIMP loops can significantly enhance our prospects for discovery by precise measurement of Standard Model processes. This study focuses on the indirect detection method within the <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>μ</mi><mi>TRISTAN</mi></math> experiment, with a specific emphasis on TeV-scale EWIMP dark matter scenarios that yield the correct thermal relic density. At collision energies for <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><msqrt><mrow><mi>s</mi></mrow></msqrt><mo>=</mo><mi>O</mi><mo stretchy=\"false\">(</mo><mn>1</mn><mi>–</mi><mn>10</mn><mo stretchy=\"false\">)</mo><mtext> </mtext><mtext> </mtext><mi>TeV</mi></mrow></math>, these EWIMPs introduce noticeable effects, typically in the range of <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>O</mi><mo stretchy=\"false\">(</mo><mn>0.1</mn><mi>–</mi><mn>1</mn><mo stretchy=\"false\">)</mo><mo>%</mo></mrow></math>. Our findings indicate that at <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>2</mn><mo stretchy=\"false\">(</mo><mn>10</mn><mo stretchy=\"false\">)</mo><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math>, with an integrated luminosity of <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mn>10</mn><mtext> </mtext><mtext> </mtext><msup><mrow><mi>ab</mi></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math>, <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>μ</mi><mi>TRISTAN</mi></math> can detect Higgsinos at a mass of 1.3 (3.0) TeV and winos at a mass of 1.9 (4.4) TeV, assuming an optimistic level of systematic uncertainty in the observation of the Standard Model processes.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"28 1","pages":""},"PeriodicalIF":5.3000,"publicationDate":"2024-08-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Indirect probe of electroweak-interacting particles at the μTRISTAN μ+μ+ collider\",\"authors\":\"Risshin Okabe, Satoshi Shirai\",\"doi\":\"10.1103/physrevd.110.035002\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A novel collider, called <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>μ</mi><mi>TRISTAN</mi></math>, was recently proposed, offering the capability to achieve high-energy collisions of antimuons. 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At collision energies for <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><msqrt><mrow><mi>s</mi></mrow></msqrt><mo>=</mo><mi>O</mi><mo stretchy=\\\"false\\\">(</mo><mn>1</mn><mi>–</mi><mn>10</mn><mo stretchy=\\\"false\\\">)</mo><mtext> </mtext><mtext> </mtext><mi>TeV</mi></mrow></math>, these EWIMPs introduce noticeable effects, typically in the range of <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>O</mi><mo stretchy=\\\"false\\\">(</mo><mn>0.1</mn><mi>–</mi><mn>1</mn><mo stretchy=\\\"false\\\">)</mo><mo>%</mo></mrow></math>. Our findings indicate that at <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>2</mn><mo stretchy=\\\"false\\\">(</mo><mn>10</mn><mo stretchy=\\\"false\\\">)</mo><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math>, with an integrated luminosity of <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mn>10</mn><mtext> </mtext><mtext> </mtext><msup><mrow><mi>ab</mi></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math>, <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>μ</mi><mi>TRISTAN</mi></math> can detect Higgsinos at a mass of 1.3 (3.0) TeV and winos at a mass of 1.9 (4.4) TeV, assuming an optimistic level of systematic uncertainty in the observation of the Standard Model processes.\",\"PeriodicalId\":20167,\"journal\":{\"name\":\"Physical Review D\",\"volume\":\"28 1\",\"pages\":\"\"},\"PeriodicalIF\":5.3000,\"publicationDate\":\"2024-08-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical Review D\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/physrevd.110.035002\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review D","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevd.110.035002","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
摘要
最近提出了一个名为μTRISTAN的新型对撞机,它能够实现反质子的高能对撞。这种高能对撞机为发现电弱相互作用大质量粒子(EWIMPs)提供了一个难得的机会,各种新物理模型都预测了这种粒子的存在。在像μTRISTAN这样的轻子对撞机中,发现EWIMPs的潜力超出了其直接产生的范围。通过对标准模型过程的精确测量,EWIMP环产生的量子修正可以大大提高我们的发现前景。本研究侧重于μTRISTAN实验中的间接探测方法,特别强调产生正确热遗迹密度的TeV尺度EWIMP暗物质方案。在 s=O(1-10) TeV 的碰撞能量下,这些 EWIMP 带来了明显的影响,通常在 O(0.1-1)% 的范围内。我们的研究结果表明,在 s=2(10) TeV、综合光度为 10 ab-1 的条件下,μTRISTAN 可以探测到质量为 1.3 (3.0) TeV 的希格斯微子和质量为 1.9 (4.4) TeV 的赢子,同时假设标准模型过程观测的系统不确定性处于乐观水平。
Indirect probe of electroweak-interacting particles at the μTRISTAN μ+μ+ collider
A novel collider, called , was recently proposed, offering the capability to achieve high-energy collisions of antimuons. This high-energy collider presents an exceptional opportunity for the discovery of electroweak-interacting massive particles (EWIMPs), which are predicted by various new physics models. In a lepton collider like , the potential for discovering EWIMPs extends beyond their direct production. Quantum corrections arising from EWIMP loops can significantly enhance our prospects for discovery by precise measurement of Standard Model processes. This study focuses on the indirect detection method within the experiment, with a specific emphasis on TeV-scale EWIMP dark matter scenarios that yield the correct thermal relic density. At collision energies for , these EWIMPs introduce noticeable effects, typically in the range of . Our findings indicate that at , with an integrated luminosity of , can detect Higgsinos at a mass of 1.3 (3.0) TeV and winos at a mass of 1.9 (4.4) TeV, assuming an optimistic level of systematic uncertainty in the observation of the Standard Model processes.
期刊介绍:
Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics.
PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including:
Particle physics experiments,
Electroweak interactions,
Strong interactions,
Lattice field theories, lattice QCD,
Beyond the standard model physics,
Phenomenological aspects of field theory, general methods,
Gravity, cosmology, cosmic rays,
Astrophysics and astroparticle physics,
General relativity,
Formal aspects of field theory, field theory in curved space,
String theory, quantum gravity, gauge/gravity duality.