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Fusion in Nuclear Physics: A Closer Look

Investigating fusion excitation functions and challenges with low-abundance isotopes.

― 5 min read


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In nuclear physics, Fusion refers to the process where two light atomic nuclei combine to form a heavier nucleus. This reaction is significant for understanding how elements are formed in stars and other cosmic events. One key aspect of studying fusion is measuring Excitation Functions, which tell us how often these fusion reactions occur at different energy levels. However, there are challenges when measuring these functions, especially for certain Isotopes that exist in very small amounts naturally.

The Challenge of Low-Abundance Isotopes

Most fusion studies focus on nuclei with significant natural abundance, which are easier to work with. For nuclei that are rare, obtaining enough material can be tough. Researchers often need isotopically enriched samples, which are difficult and costly to produce. This limitation means that there are gaps in our knowledge about how fusion behaves in less common isotopes. This is particularly true for neutron-rich nuclei, which can have interesting properties that affect how they behave in fusion reactions.

Thick-Target Techniques

To overcome the problems faced with low-abundance beams, one approach is to use thick-target techniques. In this method, a thicker target is used, allowing researchers to conduct measurements even with lower intensity beams. This is essential because conventional methods often require beams that are strong enough to penetrate a simple target. By using a thick target, researchers can measure how often fusion occurs with less intense isotopes.

Active Thick-Target Approach

A specific type of thick-target technique is the active thick-target approach. This involves using a detector that can actively register the products of fusion as they happen. One such detector is called MuSIC, which is designed to measure the energy lost by particles as they pass through it. When a fusion event occurs, the resulting compound nucleus produces particles that have different energy levels, allowing researchers to track and measure these reactions accurately.

How MuSIC Works

The MuSIC detector consists of an ionization chamber that captures the energy from incoming particles. It has a design that allows it to measure energy very precisely, which is crucial for understanding the details of fusion processes. As the particles pass through the chamber, they lose energy, and the detector records this energy loss. If fusion takes place, the resulting particles can be identified based on their increased energy, distinguishing them from the original beam particles.

Calibration and Measurements

Calibration is a vital part of using the MuSIC detector, as it ensures that the measurements taken are accurate. This is done by firing known particles into the detector and measuring the energy they lose, allowing adjustments to be made for future measurements. This method brings forth an efficient way to gather data on how fusion functions at various energy levels.

Importance of Accurate Measurements

Conducting accurate measurements of fusion processes is crucial for expanding our understanding of nuclear structure and reactions. By studying different isotopes, particularly the less abundant ones, researchers can observe patterns and behaviors that significantly contribute to nuclear physics. Low-intensity beams can be challenging, but with advanced techniques, scientists can gather reliable data that fills gaps in existing knowledge.

The Case of Oxygen and Carbon Fusion

One notable study involved measuring the fusion excitation function of oxygen nuclei colliding with carbon targets. Research found significant interest in how these events occur, particularly at certain energy levels. By using the MuSIC detector with a low-intensity oxygen beam, researchers were able to compare their results with previous data, revealing new insights about the fusion cross-section at different energies.

Comparing Results with Other Reactions

The findings from the fusion of oxygen with carbon were compared to similar reactions involving fluorine and carbon. Since these two nuclei are mirror nuclei, a similar behavior in the fusion process is expected. Researchers looked at the differences in energy levels and how the fusion excitation functions matched up. This comparison is essential for validating the accuracy of measurements and understanding nuclear interactions.

Exploring Neutron-Rich Nuclei

Studying neutron-rich nuclei is particularly fascinating because they can display unique properties not found in more stable isotopes. Researchers are keen to identify trends in fusion behavior when examining how neutron excess affects these reactions. By mapping the average fusion cross-section for different isotopes in various energy ranges, scientists can build a clearer picture of how these reactions work.

Insights into Neutron Pairing Effects

The measurement of fusion cross-sections also helps in understanding pairing effects among neutrons. In nuclear physics, pairing refers to how neutrons group together in certain configurations, which can influence the likelihood of fusion. By analyzing the fusion of various isotopes, particularly those that are neutron-rich, researchers can unravel some of the complexities associated with these pairing effects.

Future Directions in Fusion Research

As technologies improve and new methods are developed, research into fusion and excitation functions will become even more precise. The use of advanced detectors like MuSIC not only enhances measurement capabilities but also opens up new avenues for research. This progress is vital for grasping the fundamental aspects of nuclear physics and for applying this knowledge to broader scientific questions, such as the formation of elements in the universe.

Conclusion

Studying fusion excitation functions is a crucial part of nuclear science that allows researchers to probe the properties of atomic nuclei. By employing techniques that enable the measurement of low-intensity beams, scientists can glean insights into the behavior of less common isotopes. As future studies build upon these findings, the knowledge gained will deepen our comprehension of nuclear reactions and the intricate science behind them.

Original Source

Title: Obtaining high resolution excitation functions with an active thick-target approach and validating them with mirror nuclei

Abstract: Measurement of fusion excitation functions for stable nuclei has largely been restricted to nuclei with significant natural abundance. Typically, to investigate neighboring nuclei with low natural abundance has required obtaining isotopically enriched material. This restriction often limits the ability to perform such measurements. We report the measurement of a high quality fusion excitation function for a $^{17}$O beam produced from unenriched material with 0.038\% natural abundance. The measurement is enabled by using an active thick-target approach and the accuracy of the result is validated using its mirror nucleus $^{17}$F and resonances. The result provides important information about the average fusion cross-section for the oxygen isotopic chain as a function of neutron excess.

Authors: S. Hudan, J. E. Johnstone, Rohit Kumar, R. T. deSouza, J. Allen, D. W. Bardayan, D. Blankstein, C. Boomershine, S. Carmichael, A. Clark, S. Coil, S. L. Henderson, P. D. O'Malley, W. W. von Seeger

Last Update: 2023-04-18 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2304.09117

Source PDF: https://arxiv.org/pdf/2304.09117

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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