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Normally we think of dark matter as only interacting via the force of gravity, but certain types should interact in other ways although weakly. A new model could indicate that one way the sun radiates heat is via a certain type of dark matter that we should be able to find in one of the various ongoing dark matter searches.
Article
Here's a shorter, less detailed article on the topic.
Article
Unexplained discrepancies between mathematical models of the Sun and astronomical observations could be resolved by the presence of dark matter in the Sun, according to the latest work from an international team of researchers. The team's model – which looks at dark matter that has a particular, momentum-dependent interaction with normal matter – explains the observed data much better than more conventional dark-matter models. The researchers believe that the particles they postulate could potentially be seen either by direct detectors or in particle accelerators.
In recent years, scientists have reduced their estimates of the proportion of elements heavier than hydrogen and helium in the Sun. These new estimates, based on reinterpretations of spectroscopic data, create a problem. When applied to conventional mathematical models of the solar structure, they create multiple conflicts with the values of various quantities that are measured by looking at periodic changes in size of the Sun caused by acoustic pressure waves. This study of the internal structure of the Sun via acoustic waves is known as helioseismology. To resolve these inconsistencies, researchers are seeking new ways that heat can reach the surface of the Sun from its core. One possibility is that the Sun might contain dark matter that it captures as it passes through the galactic halo. Such matter could carry heat from the core to the cooler outer layers of the Sun.
Here's a shorter, less detailed article on the topic.