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Probing CP violation in dark scalar decays at the SHiP experiment

This paper proposes using the SHiP experiment to probe CP violation in GeV-scale dark scalar bosons by analyzing the ratio of three-meson to two-meson decay events, which arise from pseudoscalar and scalar couplings respectively, alongside complementary two-muon and di-photon channels.

Original authors: Mayumi Aoki, Takashi Shimomura

Published 2026-10-09
📖 5 min read🧠 Deep dive

Original authors: Mayumi Aoki, Takashi Shimomura

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). ✨ This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

In the vast, invisible landscape of the universe, there is a persistent mystery that the known laws of physics cannot fully explain: why does the cosmos contain more matter than antimatter? According to our current understanding, the Big Bang should have created equal amounts of both, which would have annihilated each other instantly, leaving behind a universe filled only with light. The fact that we exist, that stars shine and planets form, suggests that something tipped the scales in favor of matter. Physicists call this imbalance a violation of a fundamental symmetry known as CP violation. While we have observed this phenomenon in a few specific, rare particle interactions, the known sources are not strong enough to account for the entire universe's existence. This gap in our knowledge has led scientists to look for new, hidden sources of this asymmetry, often theorizing the existence of a "dark sector"—a realm of particles that interact very weakly with the ordinary matter we see every day.

One promising candidate for a resident of this dark sector is a dark scalar boson, a type of particle that is invisible to our eyes but could be produced in high-energy collisions. If such a particle exists, it might be a "mixture" of two different states: one that behaves like a mirror image of itself and one that does not. Determining whether this particle is a pure mirror image, a pure non-mirror image, or a blend of both is crucial. If it is a blend, it would be direct evidence of a new kind of CP violation, potentially solving the mystery of why the universe is made of matter. However, because these particles interact so weakly, they are incredibly difficult to catch, and their behavior is subtle.

A team of researchers has proposed a clever way to hunt for this specific type of particle using two upcoming experiments designed to catch long-lived particles: SHiP, located at CERN in Europe, and FASER2, situated at the Large Hadron Collider. The researchers focused on a dark scalar boson with a mass roughly between one and two billion electron volts, a scale that is heavy enough to be interesting but light enough to be produced in large numbers. Their strategy relies on watching how this invisible particle decays, or falls apart, into other, more familiar particles. The key insight is that the way the particle breaks apart depends entirely on its internal nature. If the particle is a pure mirror-image state, it will almost exclusively break apart into pairs of mesons, which are particles made of a quark and an antiquark. If it is a pure non-mirror state, it will almost exclusively break apart into groups of three mesons.

The researchers realized that if the dark scalar is a mixture of both states, it would be a smoking gun for new physics. In this scenario, the particle would decay into both pairs and triplets of mesons simultaneously. To test this, the team simulated the conditions of the SHiP and FASER2 experiments, calculating how many of these particles would be produced from the decay of heavier B-mesons and how many would survive long enough to reach the detectors. They found that for a wide range of possible masses and mixing angles, the experiments would see a significant number of events where the dark scalar decays into two mesons, and a separate, distinct number of events where it decays into three mesons. By comparing the ratio of these two types of events, scientists could determine the exact nature of the dark scalar's CP violation.

The study also looked at other ways the particle might decay, such as into pairs of muons or pairs of photons. While these channels are also useful, the researchers found that the comparison between the two-meson and three-meson channels offers the most sensitive probe. Their simulations suggest that if the dark scalar exists with the properties they modeled, the SHiP experiment, which is designed to be exceptionally sensitive, could observe thousands of these decay events. Even if the particle interacts slightly more weakly than their most optimistic estimate, the signal would still be strong enough to distinguish between a pure state and a mixed state. The FASER2 experiment, while smaller and seeing fewer events, could still contribute valuable data, particularly for particles with masses around the mass of a specific meson called the eta-prime.

What makes this approach particularly powerful is that it does not rely on measuring complex angles or subtle correlations that require perfect detector precision. Instead, it relies on a simple count: are there particles breaking into twos, and are there particles breaking into threes? If the answer is yes to both, it proves the dark scalar is a CP-mixed state. The researchers confirmed that this signal would stand out clearly against the background noise expected in these experiments. They also checked that their conclusions held true even if the particle did not interact with electrons or muons, a scenario that would change how long the particle lives before decaying. In all cases, the ratio of the decay modes remained a reliable indicator.

This work provides a clear roadmap for the next generation of particle physics experiments. It moves beyond the theoretical possibility of a dark sector to a concrete, testable prediction. If the dark scalar boson is discovered, the very first question will be to determine its identity. By simply counting the number of particle pairs versus particle triplets in the debris of a collision, scientists will be able to answer whether this hidden particle holds the key to the universe's matter-antimatter imbalance. The proposed method turns the complex problem of quantum symmetry into a straightforward counting exercise, offering a realistic path to uncovering one of the deepest secrets of the cosmos.

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