International Workshop on Baryon and Lepton Number Violation (BLV 2024)

Europe/Berlin
Pavel Fileviez Perez (CWRU), Thomas Schwetz-Mangold (KIT)
Description

The 2024 International Workshop on Baryon and Lepton Number Violation (BLV2024) will be organized by the Institute for Astroparticle Physics at the Karlsruhe Institute of Technology (KIT), and take place in Karlsruhe on October 8-11, 2024 at KIT Campus South.

After Berkeley (2007), Madison (2009), Gattinburg (2011), Heidelberg (2013), UMass (2015), Cleveland (2017), Madrid (2019) and Brussels (2022) this will be the 9th edition of this workshop.

The main topics of this workshop are:

  • Neutrino physics
  • Baryogenesis mechanisms
  • Baryon number violating processes
  • Lepton number violation in low energy processes
  • Lepton flavor violating processes
  • Baryon and lepton number violation at colliders
  • Dark matter

and it covers a wide range of BSM physics, with both a theoretical and an experimental component.

The preliminary schedule for the conference is to start on Tue, 8 Oct 2024, 9:00 and end on Fri, 11 Oct 2024 at lunch time. We will offer the possibility to  visit the KATRIN neutrino mass experiment on Friday afternoon. There is no conference fee.

Oral contributions are by invitation only, but we welcome abstract submissions for contributed talks (subject to approval), especially for early career researchers. Abstract submission deadline is 30 June 2024.

WARNING: if you get contacted by an "agency" or "company" offering some services related to your participation, please do not reply and ignore such messages.  They are scam, we have not engaged any company related to BLV2024.

This workshop is supported by the KIT Center Elementary Particle and Astroparticle Physics (KCETA) and by the Collaborative Research Center Particle Physics Phenomenology after the Higgs Discovery

Picture: Karlsruhe Castle @ Night – © Stefan Zimmermann

General Terms and Conditions of KIT for the Registration for Events

 

Participants
  • Alejandro Ibarra
  • Ana M. Teixeira
  • Bahaa Ilyas
  • Camilo Alfredo García Cely
  • Chui-Fan Kong
  • Daniel Naredo
  • David Milstead
  • Felix Kahlhoefer
  • Francesco D'Eramo
  • Giovani Dalla Valle Garcia
  • Giovanni Dal Maso
  • Gonzalo Herrera
  • Herbert Dreiner
  • HOOMAN DAVOUDIASL
  • Jelle Groot
  • Jing-Yu Zhu
  • John Gargalionis
  • Jonathan Kriewald
  • Joscha Lauer
  • Jose Cuenca Garcia
  • Julia Harz
  • Julian Günther
  • Julian Heeck
  • Julieta Gruszko
  • Juri Smirnov
  • Kevin Alberto Urquía Calderón
  • Kevin Gonzalez Quesada
  • Kierthika Chathirathas
  • Kiran Sharma
  • Laura Lopez Honorez
  • Lisa Biermann
  • Maksym Ovchynnikov
  • Marieke Postma
  • Martin Mojahed
  • Michal Malinský
  • Michele Frigerio
  • Michele Maltoni
  • Miha Nemevšek
  • Nicolas Perez
  • Nuria Rius
  • Oleksii Mikulenko
  • OSCAR PASTOR
  • Pavel Fileviez Perez
  • Peter Maták
  • Prativa Pritimita
  • Praveen Bharadwaj
  • Rebeca Beltrán
  • Renata Zukanovich Funchal
  • René Reimann
  • Riccardo Fantechi
  • Richard Ruiz
  • Rishav Roshan
  • Robert Ziegler
  • Sabya Sachi Chatterjee
  • Sangeeta Dey
  • Sascha Weber
  • Silvia Pascoli
  • Soumen Kumar Manna
  • Stefan Antusch
  • Stefan E. Müller
  • Stefan Vogl
  • Thomas Rink
  • Thomas Schwetz-Mangold
  • Tim Kretz
  • Vaisakh Plakkot
  • Volodymyr Takhistov
  • Yohei Ema
  • Youngjoon Kwon
  • Yuber F Perez-Gonzalez
    • 9:00 AM 9:15 AM
      Welcome
    • 9:15 AM 10:45 AM
      Baryon number violating processes: 1
      • 9:15 AM
        Hyperkamiokande (25'+5') 30m
        Speaker: Volodymyr Takhistov (QUP, KEK)
      • 9:45 AM
        Recent Theory Developments on Baryon Number Violating Processes in the Context of GUTs (25'+5') 30m
        Speaker: Michal Malinský (IPNP, Charles University, Prague)
      • 10:15 AM
        Recent Experimental Activities in Neutron-Antineutron Oscillations (25'+5') 30m
        Speaker: David Milstead (Fysikum, Stockholms Universitet)
    • 10:45 AM 11:15 AM
      Coffee break 30m
    • 11:15 AM 12:50 PM
      Baryon number violating processes: 2
      • 11:15 AM
        Baryon Number Violation EFT (20'+5') 25m
        Speaker: John Gargalionis (IFIC)
      • 11:40 AM
        Destabilizing Matter through a Long-Range Force (20'+5') 25m
        Speaker: HOOMAN DAVOUDIASL (Brookhaven National Laboratory)
      • 12:05 PM
        Dark Matter Catalyzed Baryon Destruction (20'+5') 25m
        Speaker: Yohei Ema
      • 12:30 PM
        Sources of CP Violation for Electroweak Baryogenesis (17'+3') 20m

        A persistent issue in electroweak baryogenesis calculations is the significant disparity in predictions yielded by different approaches, with variations spanning several orders of magnitude. In this study, we examine a system comprising two fermion flavours, proposing the existence of two sources of CP-violating. The semiclassical force and a new resonantly enhanced mixing source can be derived from the collisionless Kadanoff-Baym equation. The two sources are derived using the semiclassical approximation and the VEV insertion approximation. A Higgsino-Bino toy model shows that the new resonantly enhanced mixing source generates sufficient asymmetry to evade EDM bounds. In addition, a ready-to-plug equation for the source is prepared so phenomenologist can use it in their favourite model.

        Speaker: Bahaa Ilyas (Technical University of Munich)
    • 12:50 PM 2:15 PM
      Lunch break 1h 25m
    • 2:15 PM 3:45 PM
      Lepton flavor violating processes: 1
      • 2:15 PM
        Lepton Flavour Violation (25'+5') 30m
        Speaker: Ana M. Teixeira (LPC Clermont)
      • 2:45 PM
        Lepton Flavor Violation by Two Units (17'+3') 20m
        Speaker: Julian Heeck (University of Virginia)
      • 3:05 PM
        The Latest Results of the MEG II Experiment (17'+3') 20m
        Speaker: Giovanni Dal Maso (Psul Sherrer Insitut - PSI)
      • 3:25 PM
        Probing CLFV with the Mu2e Experiment at Fermilab (17'+3') 20m
        Speaker: Stefan E. Müller (Helmholtz-Zentrum Dresden-Rossendorf)
    • 3:45 PM 4:15 PM
      Coffee break 30m
    • 4:15 PM 6:00 PM
      Lepton flavor violating processes: 2
      • 4:15 PM
        Search for LFV and Light New Physics at Belle-II (17'+3') 20m
        Speaker: Youngjoon Kwon (Department of Physics, Yonsei University)
      • 4:35 PM
        Searches for Hidden Sectors and Lepton Flavour Violation in Kaon Decays (17'+3') 20m

        Rare kaon decays are among the most sensitive probes of both heavy and light new physics beyond the Standard Model description thanks to high precision of the Standard Model predictions, availability of very large datasets, and the relatively simple decay topologies. The NA62 experiment at CERN is a multi-purpose high-intensity kaon decay experiment, and carries out a broad rare-decay and hidden-sector physics programme. NA62 has collected a large sample of $K^+$ decays in flight during Run 1 in 2016-2018, and the ongoing Run 2 which started in 2021. Recent NA62 results on searches for hidden-sector mediators and searches for violation of lepton number and lepton flavour conservation in kaon decays based on the Run 1 dataset are presented. Future prospects of these searches are discussed.

        Speaker: Riccardo Fantechi (INFN - Sezione di Pisa)
      • 4:55 PM
        Bounds on Ultra Heavy HNLs (17'+3') 20m

        Heavy Neutral Leptons (HNLs) are hypothetical particles that are able to explain neutrino oscillations. The presence of HNLs induces charged lepton flavor violating (cLFV) processes. Non-observations of these processes puts the strongest limits on parameters of HNL much heavier than the electroweak scale.
        We demonstrate that for such HNLs, the branching ratio of cLFV processes is actually mass-dependent. Given this fact, we improve current bounds on HNL mass and mixing angle. Furthermore, we perform a perturbative unitarity analysis to identify the domain of validity of our results.

        Speaker: Mr Kevin Alberto Urquía-Calderón (Niels Bohr Institute)
      • 5:15 PM
        Heavy Sterile Neutrinos from B decays and new QCD Corrections to their Semi-Hadronic Decay Rates (17'+3') 20m

        In modern experiments on flavour physics it is possible to search for the decays of $B$’s, $D$’s, or $\tau$’s into final states with heavy neutrinos $N$ (a.k.a. heavy neutral leptons). I present a common study of theorists and experimentalists from Belle II on constraints on $B-> D^{*} \ell N$. Next I discuss the status of the theory predictions of the various $N$ decay rates. In scenarios in which $N$ interacts with SM particles only through sterile-active neutrino mixing, the dependence of the lifetime on the relevant mixing angles is important to determine whether $N$ decays in the detector or outside. To calculate the inclusive decay rate into semi-hadronic final states reliably one needs to include radiative QCD corrections. I present analytic results for the QCD-corrected decay rates and discuss their phenomenological impact.

        Speaker: Mr Tim Kretz (Karlsruher Institut für Technologie (KIT - TTP))
      • 5:35 PM
        Testing the Standard Model with Most Accurate Muon g-2 Measurements (17'+3') 20m

        The magnetic moment anomaly of the muon, that relates the cyclotron and spin precession frequency, provides one of the most stringent tests of the Standard Model of Particle Physics since it is measured and theoretically predicted to very high precision. Deviations between theoretical prediction and experimental measurements can be used to investigate tensions in the methods or can be interpreted as hints for physics beyond the Standard Model. In August 2023, the Fermilab Muon g-2 experiment reported its result from measurement campaigns 2 and 3, which in combination with run 1 increased the precision to now 200 ppb. The increase in precision is both due to increased statistics and reduced systematics. This milestone puts the Muon g-2 experiment well on its way to surpass its design precision of 140 ppb with final statistics. In this contribution we review the measurement principle of the Muon g-2, point out experimental improvements in the recent measurement and put the measurement in the context of the current theoretical effort.

        Speaker: René Reimann (Johannes Gutenberg University, Mainz)
    • 6:00 PM 8:00 PM
      Welcome reception 2h
    • 9:00 AM 10:35 AM
      B and L violation at current or future colliders: 1
      • 9:00 AM
        Heavy Neutrino-Antineutrino Oscillations at Collider Experiments (25'+5') 30m
        Speaker: Stefan Antusch (University of Basel)
      • 9:30 AM
        Prospects for Discovering LNV at the FCC (20'+5') 25m

        Whether lepton number is a conserved or violated symmetry of nature remains one of the most pressing questions today, with far-reaching consequences across astrophysics, particle physics, and nuclear physics. If lepton number is indeed violated, it is also unknown whether it occurs at a scale accessible with laboratory experiments. The discovery of lepton number violation in the laboratory would have a monumental impact on understanding what lies beyond the Standard Model of Particle Physics. This talk gives a broad overview of the (current) projected sensitivity to discovering lepton number violation at the proposed Future Circular Collider program at CERN.

        Speaker: Richard Ruiz (IFJ PAN)
      • 9:55 AM
        On Lepton Number Violation in Type II Seesaw (17'+3') 20m

        We determine the prospect of observing genuine lepton number violating (LNV) signals at hadron
        colliders in the context of type II seesaw.
        The model features smoking gun signals with same-sign di-leptons and jets that may be the
        primary observable channel in a certain portion of parameter space.
        The charged lepton flavour composition in the minimal model relates to the origin of neutrino mass
        and correlates with other rare processes, such as neutrinoless double beta decay.
        We review the existing collider limits and provide sensitivity estimates of LNV signals, with
        degenerate masses and with mass splittings, for the upcoming runs at the LHC.

        Speaker: Jonathan Kriewald (IJS)
      • 10:15 AM
        Some Novel Searches for Neutrino Dipole Moments (17'+3') 20m
        Speaker: Michele Frigerio
    • 10:35 AM 11:05 AM
      Coffee break 30m
    • 11:05 AM 12:40 PM
      Baryogenesis mechanisms: 1
      • 11:05 AM
        Observable Leptogenesis (25'+5') 30m
        Speaker: Nuria Rius (IFIC, CSIC-Valencia University)
      • 11:35 AM
        Wash-in Leptogenesis with Dirac Neutrino Scatterings (20'+5') 25m

        We present a Dirac leptogenesis model in which the only out-of-equilibrium particles are right-handed neutrinos undergoing asymmetric scatterings. They are produced from a negligible initial abundance and their density freezes in soon after reheating. Even though the asymmetry source term vanishes, we demonstrate that opposite asymmetries of right-handed neutrinos and standard model leptons are washed in.

        Speaker: Peter Maták (Comenius University in Bratislava)
      • 12:00 PM
        Effects of Reheating on Charged Lepton Yukawa Equilibration and Leptogenesis (17'+3') 20m

        We show that the process of non-instantaneous reheating during the post-inflationary period can have a sizable impact on the charged lepton Yukawa equilibration temperature in the early Universe. This suggests relooking the effects of lepton flavors in the leptogenesis scenario where the production and decay of right-handed neutrinos take place within this prolonged era of reheating. We find this observation has the potential to shift the flavor regime(s) of leptogenesis compared to the standard thermal scenario.

        Speaker: Dr Rishav Roshan (University Of Southampton)
      • 12:20 PM
        Spontaneous Leptogenesis with sub-GeV Axion Like Particles (17'+3') 20m

        A derivative coupling of an axion-like particle (ALP) with a B-L current can lead to the baryon asymmetry of the universe through spontaneous leptogenesis, provided there is a lepton number-breaking interaction in thermal equilibrium. Typically, this requires heavy ALPs and a high reheating temperature, as the lepton number-breaking is also linked to neutrino mass generation. In this study, we propose leveraging an inert Higgs doublet to facilitate the lepton number-violating operator, reducing this constraint. This enables the generation of lepton asymmetry (via freeze-in/out processes) at a much lower reheating temperature, accommodating light (sub-GeV) ALPs that are sensitive to current and future ALP searches.

        Speaker: Soumen Kumar Manna (Indian Institute of Technology Guwahati)
    • 12:40 PM 2:00 PM
      Lunch break 1h 20m
    • 2:00 PM 3:35 PM
      Neutrino physics: 1
      • 2:00 PM
        Global Analysis of Oscillation Data in the Presence of BSM Neutrino Properties (25'+5') 30m
        Speaker: Michele Maltoni (Instituto de Fisica Teorica UAM/CSIC)
      • 2:30 PM
        Neutrino Mass Ordering (20'+5') 25m
        Speaker: Prof. Renata Zukanovich Funchal
      • 2:55 PM
        Probing the Neutrino Mass and Beyond with the KATRIN Experiment (17'+3') 20m

        The Karlsruhe Tritium Neutrino (KATRIN) experiment aims to measure the effective electron antineutrino mass using ultra-high precision spectroscopy of tritium $\beta$-decay in the kinematic endpoint region. The most stringent upper limit on the neutrino mass was recently placed at $m_\nu c^2 < 0.45\,\mathrm{eV}$ ($90\,\%$ CL), using a fraction of the final dataset and improved operational conditions.
        Processes that impact the decay kinematics or alter the interaction structure can cause spectral features beyond the neutrino mass. KATRIN investigates new physics scenarios such as mixing with an eV-scale sterile neutrino, the capture of cosmic relic neutrinos on tritium nuclei, and signatures of Lorentz-invariance violation. Additionally, the experiment probes non-standard interactions contributing in the decay structure and explores the coupling of eV-scale BSM bosons to the final state leptons.
        This talk will review the latest result of KATRIN and present a selection of the aforementioned searches beyond the neutrino mass.

        Speaker: Joscha Lauer (KIT)
      • 3:15 PM
        Is Cosmology in Conflict with Neutrino Oscillations? (17'+3') 20m
        Speaker: Daniel Naredo (IFT-UAM/CSIC)
    • 3:35 PM 4:05 PM
      Coffee break 30m
    • 4:05 PM 5:25 PM
      Neutrino physics: 2
      • 4:05 PM
        Boosting the Production of Sterile Neutrino Dark Matter with Self-Interactions (17'+3') 20m

        Sterile neutrinos are well-motivated and simple dark matter (DM) candidates. However, sterile neutrino DM produced through oscillations by the Dodelson-Widrow mechanism is excluded by current X-ray observations and bounds from structure formation. One minimal extension, that preserves the attractive features of this scenario, is self-interactions among sterile neutrinos. In this work, we analyze how sterile neutrino self-interactions mediated by a scalar affect the production of keV sterile neutrinos for a wide range of mediator masses. We find four distinct regimes of production characterized by different phenomena, including partial thermalization for low and intermediate masses and resonant production for heavier mediators. We show that significant new regions of parameter space become available which provide a target for future observations.

        Speaker: Stefan Vogl
      • 4:25 PM
        New Physics and Primordial Neutrinos Decoupling: a DSMC Approach (17'+3') 20m

        Primordial neutrinos are important messengers from the Early Universe, affecting several key observables such as primordial nuclear abundances and cosmic microwave background. If some new physics existed at the time around neutrino decoupling, it would have left imprints on the neutrino distribution function, which requires solving the neutrino Boltzmann equation. Existing approaches have limitations that prevent using them in a universal way for the cases with new physics particles decaying into neutrinos. Addressing this issue, we present a novel approach to studying the interactions of neutrinos based on Direct Simulation Monte Carlo (DSMC). In particular, we resolve the existing discrepancies between the Boltzmann codes regarding the impact of highly non-thermal neutrinos on Neff, and study the interplay of possible large lepton asymmetries in the neutrino sector and injections of high-energy neutrinos.

        Speaker: Maksym Ovchynnikov (Karlsruhe Institute of Technology)
      • 4:45 PM
        Long-lived Neutral Fermions at the DUNE near Detector (17'+3') 20m

        At the Deep Underground Neutrino Experiment (DUNE), a proton beam hits a fixed target leading to large production rates of mesons. These mesons can decay and potentially provide a source of long-lived neutral fermions. Examples of such long-lived fermions are heavy neutral leptons which can mix with the standard-model active neutrinos, and the bino-like lightest neutralino in R-parity-violating supersymmetry. We show that the Standard Model Effective Field Theory extended with right-handed singlet neutrinos can simultaneously describe heavy neutral leptons and bino-like neutralinos in a unified manner. We use the effective-field-theory framework to determine the sensitivity reach of the DUNE near detector in probing various scenarios of long-lived neutral fermions.

        Speaker: Julian Günther (Universität Bonn)
      • 5:05 PM
        Testing Neutrino Mass Origins with Supernova Neutrinos (17'+3') 20m
        Speaker: Chui-Fan Kong
    • 9:00 AM 10:45 AM
      Dark Matter: 1
      • 9:00 AM
        Matter-Antimatter Asymmetry and Dark Matter Stability from Baryon Number Conservation (25'+5') 30m
        Speaker: Alejandro Ibarra (Technical University of Munich)
      • 9:30 AM
        Cosmic Axion Background from the Primordial Bath (20'+5') 25m
        Speaker: Francesco D'Eramo (University of Padua & INFN Padua)
      • 9:55 AM
        Dark Matter Decay (20'+5') 25m
        Speaker: Laura Lopez-Honorez
      • 10:20 AM
        Axion Haloscopes for Gravitational Wave Searches (20'+5') 25m
        Speaker: Dr Camilo Garcia Cely
    • 10:45 AM 11:15 AM
      Coffee break 30m
    • 11:15 AM 12:35 PM
      Dark Matter: 2
      • 11:15 AM
        Strongly-Interacting Massive Particles and Dark Matter Capture in Celestial Bodies (17'+3') 20m
        Speaker: Juri Smirnov (University of Liverpool)
      • 11:35 AM
        Direct Detection of Light DM (17'+3') 20m
        Speaker: Gonzalo Herrera (Virginia Tech)
      • 11:55 AM
        Gamma Lines and Dark Matter from Anomaly Cancellation (17'+3') 20m

        We discuss a simple theory for physics beyond the Standard Model where a Majorana dark matter is predicted from anomaly cancellation. We discuss in detail the minimal theory where the baryon number is a local symmetry spontaneously broken at the low scale. The correlation between the cosmological constraints on the dark matter relic density, the direct detection and collider bounds is investigated. We discuss in great detail the gamma lines from dark matter annihilation showing the possibility to test these predictions in the near future at gamma-ray telescopes such as CTA. We investigate all processes contributing to the total photon flux from dark matter annihilation and point out the unique features that can be used to test this theory for dark matter.

        Speaker: Kevin Gonzalez Quesada (Case Western Reserve University)
      • 12:15 PM
        Not-so-inelastic Dark Matter (17'+3') 20m

        Models of inelastic (or pseudo-Dirac) Dark Matter (DM) commonly assume an accidental symmetry between the left-handed and right-handed mass terms in order to suppress diagonal couplings. We point out that this symmetry is unnecessary, because for Majorana fermions the diagonal couplings are not strongly constrained. Removing the requirement of such an accidental ad-hoc symmetry instead relaxes the relic density constraint due to additional annihilation modes.

        In the talk, I will introduce a simple UV-complete model realizing the new asymmetric set-up. Then, I will explain how traditional constraints from (in)direct detection, beam dump experiments and colliders are modified indicating two viable mass regions for the DM particle, around a few hundred MeV and around a few GeV. The former region will be fully tested by near-future analyses of NA64 and Belle II data, while the latter turns out to be challenging to explore even with future experiments.

        Speaker: Giovani Dalla Valle Garcia (IAP - KIT)
    • 12:35 PM 2:00 PM
      Lunch break 1h 25m
    • 2:00 PM 3:40 PM
      Baryogenesis mechanisms: 2
      • 2:00 PM
        Electroweak Baryogenesis (25'+5') 30m
        Speaker: Marieke Postma (Nikhef, Amsterdam, Netherlands)
      • 2:30 PM
        Tracking Minima, Phase Transitions and Gravitational Waves with BSMPTv3 (17'+3') 20m
        Speaker: Lisa Biermann (Institute for Theoretical Physics, Karlsruhe Institute of Technology)
      • 2:50 PM
        Gravitational Particle Production and Leptogenesis (25'+5') 30m
        Speaker: Yuber F Perez-Gonzalez (IPPP, Durham University)
      • 3:20 PM
        Impact of Non-Standard Interactions on Low-Scale Leptogenesis and Neutrinoless Double Beta Decay (17'+3') 20m

        In this talk, we investigate the interplay between the observation of lepton number violating processes and the generation of the baryon asymmetry of the Universe via low-scale leptogenesis. We focus on the impact of non-standard interactions, beyond the usual Majorana mass term, on the observation of neutrinoless double beta decay and the resulting parameter space for successful leptogenesis. Parameterizing these effects in a model independent way, we showcase how additional operators can influence the final baryon asymmetry.

        Speaker: Sascha Weber (JGU Mainz)
    • 3:40 PM 4:10 PM
      Coffee break 30m
    • 4:10 PM 5:40 PM
      B and L violation at current or future colliders: 2
      • 4:10 PM
        Review of Left-Right Symmetry and its Experimental Signatures (25'+5') 30m
        Speaker: Miha Nemevšek (Jožef Stefan Institute)
      • 4:40 PM
        Quasi-Dirac HNLs in the Left-Right Symmetric Model (17'+3') 20m

        A quasi-Dirac pair of Heavy Neutral Leptons possesses a number of features that make it an appealing target for search in the GeV mass scale at future collider experiments. This scenario is studied in the Left-Right Symmetric Model. Predictions for the HNL couplings to different lepton flavors are derived, and the possible probes of the model based on the LNV signature are considered.

        Speaker: Oleksii Mikulenko (Leiden University)
      • 5:00 PM
        Probing Light Sterile Neutrinos in Left-Right Symmetric Models with Displaced Vertices and Neutrinoless Double Beta Decay (17'+3') 20m

        An investigation of relatively light (GeV-scale), long-lived right-handed neutrinos is performed within minimal left-right symmetric models using the neutrino-extended Standard Model Effective Field Theory framework. Light sterile neutrinos can be produced through rare decays of kaons, $D$-mesons, and $B$-mesons at the Large Hadron Collider (LHC) and the Long-Baseline Neutrino Facility (LBNF) of Fermilab. Their decays could result in displaced vertices, which can be reconstructed. By performing Monte-Carlo simulations, we assess the sensitivities of the future LHC far-detector experiments ANUBIS, CODEX-b, FACET, FASER(2), MoEDAL-MAPP1(2), MATHUSLA, the recently approved beam-dump experiment SHiP, and the upcoming neutrino experiment DUNE at the LBNF, to the right-handed gauge-boson mass $M_{W_R}$ as functions of neutrino masses. We find that DUNE and SHiP could be sensitive to right-handed gauge-boson masses up to $\sim 25$ TeV. We compare this reach to indirect searches such as neutrinoless double beta decay, finding that displaced-vertex searches are very competitive.

        Speaker: Jelle Groot (University of Amsterdam)
      • 5:20 PM
        Left-Right Symmetric Model with Double Seesaw Mechanism: Its LNV and LFV Imprints (17'+3') 20m
        Speaker: Prativa Pritimita (Indian Institute of Science, Bangalore)
    • 9:00 AM 9:25 AM
      Baryon number violating processes: 3
    • 9:25 AM 10:35 AM
      Lepton number violation in low energy processes: 1
      • 9:25 AM
        Review of Neutrinoless Double Beta-Decay Experiments (25'+5') 30m
        Speaker: Julieta Gruszko (UNC Chapel Hill/TUNL)
      • 9:55 AM
        Exploring neutrinoless double beta decay with the DARWIN observatory (17'+3') 20m
        Speaker: Dr Jose Cuenca Garcia (University of Zurich)
      • 10:15 AM
        Neutrinoless double-beta decay phenomenology (17'+3') 20m
        Speaker: Jing-Yu Zhu
    • 10:35 AM 11:05 AM
      Coffee break 30m
    • 11:05 AM 12:05 PM
      Lepton number violation in low energy processes: 2
      • 11:05 AM
        Lepton Number Violation and Neutrino Masses in $N_R$SMEFT (17'+3') 20m

        In this talk, we discuss tree-level UV completions for dimension 6 and 7 operators in the Standard Model Effective Field Theory extended with right-handed neutrinos ($N_R$SMEFT). We reveal that every model generating lepton number violating (LNV) operators with right-handed neutrinos also leads to the formation of active neutrino masses. This intrinsic connection between LNV processes and the existence of Majorana masses for SM neutrinos allows us to derive constraints on dimension 7 operators from the observed neutrino masses. Importantly, we demonstrate that these operators may not always be suppressed, suggesting their potential observability in future experiments.

        Speaker: Rebeca Beltrán (IFIC - University of Valencia and CSIC (Spain))
      • 11:25 AM
        Hunting for Two Right-Handed Neutrinos at Low Scales (17'+3') 20m

        The addition of two gauge singlet right-handed neutrinos to the Standard Model is a minimal extension that can potentially solve multiple open questions at once, including the observed neutrino masses via the Type-I seesaw mechanism, and the baryon asymmetry of the universe via leptogenesis. We show that combining the constraints from low-scale leptogenesis and the current non-observation of neutrinoless double beta decay ($0\nu\beta\beta$) proves to be a powerful complement to the limits obtained from Big Bang Nucleosynthesis and collider searches in order to constrain the masses and mixings of heavy neutrinos. Improved limits on $0\nu \beta\beta$ from next-generation experiments will restrict the allowed parameter space to narrow bands in the mass-mixing plane in case of inverted neutrino mass ordering, which could be probed by future collider programs, making such models with MeV-GeV range heavy neutrinos fully testable.

        Speaker: Vaisakh Plakkot
      • 11:45 AM
        Searching for LNV in Rare Meson Decays (17'+3') 20m

        We investigate the possibility of disentangling different new physics contributions to the rare meson decays $K\rightarrow\pi+$invisible and $B\rightarrow K(K^*)+$invisible through kinematic distributions in the missing invariant mass squared. We employ dimension-$6$ operators within the Low-Energy Effective Field Theory (LEFT), identifying the invisible part of the final state as either active or sterile neutrinos. Special emphasis is given to lepton-number violating (LNV) operators. We show analytically that contributions from vector, scalar, and tensor quark currents can be uniquely determined from experimental data of kinematic distributions. As there could a priori also be new invisible particles in the final states, we include dark-sector operators giving rise to two dark scalars, fermions, or vectors in the final state. We show that careful measurements of kinematic distributions make it theoretically possible to disentangle the contribution from LEFT operators from most of the dark-sector operators, even when multiple operators are contributing. Finally, we point out that an excess in rare meson decays consistent with a LNV hypothesis would point towards highly flavor non-democratic physics in the UV, and could put high-scale leptogenesis under tension.

        Speaker: Martin Mojahed (JGU/ TUM)
    • 12:05 PM 12:35 PM
      Concluding Talk (25'+5') 30m
      Speaker: Prof. Silvia Pascoli
    • 12:35 PM 2:00 PM
      Lunch break 1h 25m
    • 2:00 PM 5:00 PM
      KATRIN excursion