Can Next-Generation Accelerators Reveal the Properties of Dark Matter?

In summary, this paper discusses how high-energy measurements at next-generation accelerators can be used to determine the properties of dark matter particles, specifically in supersymmetry models with neutralino dark matter. It also highlights the important role that the proposed International Linear Collider (ILC) is expected to play in this study.
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http://arxiv.org/abs/hep-ph/0602187

Authors: Edward A. Baltz, Marco Battaglia, Michael E. Peskin, Tommer Wizansky
Comments: 121 pages, 62 figures
Report-no: SLAC-PUB-11687, LBNL-59634

If the cosmic dark matter consists of weakly-interacting massive particles, these particles should be produced in reactions at the next generation of high-energy accelerators. Measurements at these accelerators can then be used to determine the microscopic properties of the dark matter. From this, we can predict the cosmic density, the annihilation cross sections, and the cross sections relevant to direct detection. In this paper, we present studies in supersymmetry models with neutralino dark matter that give quantitative estimates of the accuracy that can be expected. We show that these are well matched to the requirements of anticipated astrophysical observations of dark matter. The capabilities of the proposed International Linear Collider (ILC) are expected to play a particularly important role in this study.
 
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This paper presents a comprehensive analysis of how high-energy measurements at next-generation accelerators might be used to determine the properties of dark matter particles, and how these measurements can be used to make predictions about the cosmic density, annihilation cross sections, and cross sections relevant to direct detection. To illustrate the capabilities of this approach, the authors focus on supersymmetry models with neutralino dark matter. They show that the expected accuracy of measurements at future accelerators is well matched to the requirements of anticipated astrophysical observations. The capabilities of the proposed International Linear Collider (ILC) are highlighted as being particularly important in this study.
 

1. What is dark matter?

Dark matter is a hypothetical form of matter that is thought to make up about 85% of the total matter in the universe. It does not interact with light and therefore cannot be observed directly. Its existence is inferred from its gravitational effects on visible matter.

2. How do scientists study dark matter at colliders?

Scientists study dark matter at colliders by using high-energy particle collisions to produce new particles, including potential dark matter particles. These collisions are recorded and analyzed to look for any unusual patterns or behaviors that may indicate the presence of dark matter.

3. What types of particles are being searched for in collider experiments?

In collider experiments, scientists are primarily searching for weakly interacting massive particles (WIMPs) as potential dark matter candidates. These particles are thought to interact with normal matter through the weak nuclear force, making them difficult to detect.

4. Has dark matter been detected at colliders?

While there have been some intriguing signals and anomalies observed at colliders that could potentially be attributed to dark matter, no conclusive detection has been made to date. Further research and experiments are ongoing to try and detect dark matter particles at colliders.

5. What are the implications of discovering dark matter at colliders?

The discovery of dark matter at colliders would have significant implications for our understanding of the universe and the fundamental laws of physics. It could provide new insights into the nature of dark matter and its role in the formation and evolution of galaxies. It could also potentially lead to the development of new technologies and applications based on our understanding of dark matter.

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