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Inverse Seesaw Neutrino Signatures at LHC and ILC

Published 16 Jul 2012 in hep-ph and hep-ex | (1207.3734v3)

Abstract: We study the collider signature of pseudo-Dirac heavy neutrinos in the inverse seesaw scenario, where the heavy neutrinos with mass at the electroweak scale can have sizable mixings with the Standard Model neutrinos, while providing the tiny light neutrino masses by the inverse seesaw mechanism. Based on a simple, concrete model realizing the inverse seesaw, we fix the model parameters so as to reproduce the neutrino oscillation data and to satisfy other experimental constraints, assuming two typical flavor structures of the model and the different types of hierarchical light neutrino mass spectra. With the fixed parameters in this way, we analyze the heavy neutrino signal at the LHC through tri-lepton final state with large missing energy and at the ILC through a single lepton plus di-jet with large missing energy. We find that in some cases, the heavy neutrino signal can be observed with a large statistical significance via different flavor charged lepton final states. Therefore, we can not only discover the heavy neutrinos in the future but also obtain a clue to reveal the origin of the small neutrino mass and flavor mixing.

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Summary

Inverse Seesaw Neutrino Signatures at LHC and ILC

The study conducted by Arindam Das and Nobuchika Okada investigates the collider signatures of pseudo-Dirac heavy neutrinos within the context of the inverse seesaw mechanism. This research proposes a theoretical framework where heavy neutrinos, possessing mass at the electroweak scale, exhibit significant mixing with the Standard Model (SM) neutrinos. This condition is pivotal as it enables the production of tiny light neutrino masses via the inverse seesaw mechanism and facilitates the potential observation of heavy neutrinos at high-energy colliders such as the Large Hadron Collider (LHC) and the International Linear Collider (ILC).

Theoretical Framework and Model

The inverse seesaw mechanism diverges from the conventional seesaw model by generating small neutrino masses through tiny lepton-number-violating parameters, rather than the suppression by a large neutrino mass scale. In this model, heavy neutrinos are treated as pseudo-Dirac particles capable of coupling with SM neutrinos through sizable Dirac Yukawa interactions. The research utilizes the next-to-minimal supersymmetric standard model (NMSSM) framework, extending it to integrate seesaw physics effectively.

The study explores two distinct flavor structure models for heavy neutrinos: the Flavor Non-Diagonal (FND) case, where the flavor structure arises from Dirac Yukawa interactions, and the Flavor Diagonal (FD) case, where it emerges from lepton-number-violating parameters. The authors assess these models under the conditions provided by SM constraints, neutrino oscillation data, and the stability of the electroweak scale.

Collider Signatures and Experimental Viability

The analysis entails scanning the parameter space to derive allowable configurations that conform with experimental constraints on the mixing matrices. Using fixed parameters, the authors perform a detailed examination of potential signals from heavy neutrino decays at the LHC and ILC. At the LHC, the prospect of observing heavy neutrino signals is investigated through tri-lepton final states and at the ILC through single lepton plus di-jet final states.

For the LHC, results indicate that while the FD flavor structure allows for significant signal observation, the FND structure results in negligible event rates. Signal events for the tri-lepton final states are calculated for both cases, yielding varying statistical significances that indicate the readiness for discovery under specific conditions.

At the ILC, studies demonstrate the potential for observing heavy neutrinos through alternative decay modes, utilizing detailed suppression techniques of SM backgrounds. The findings suggest that the inverse seesaw mechanism's predictions are observable given the assumed experimental collaboration conditions.

Future Prospects and Implications

The paper concludes that should heavy neutrinos be discovered through these proposed mechanisms, it could imply a deviation from conventional seesaw theories of neutrino mass generation. Such findings would provide new insights into the flavor structure of models for neutrino mass generation. Further research could delve deeper into optimizing detection methodologies at these colliders, potentially increasing the signal significance and exploring broader parameter space beyond the limits of this study.

The implications of this research extend into further understanding the fundamental nature of neutrinos and their interaction with SM particles. Future exploration could also focus on integrating similar mechanisms into other extensions of the standard model, thereby enhancing the scope and viability of detecting such neutrino signatures in various experimental setups.

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