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Decay pion spectroscopy of electro-produced light Lambda hypernuclei at MAMI

ORAL · Invited

Abstract

The hypertriton 3ΛH, the lightest hypernucleus, consists of a proton, a neutron, and a Lambda. This simplest Lambda hypernucleus has been used as an essential benchmark of hypernuclear physics, including understanding Λ-N interaction. Its Lambda-binding energy (BΛ) is approximately 130 ± 50 keV based on emulsion data summarized by Jurič et al. The shallow binding energy suggests a 3ΛH lifetime similar to that of a Lambda particle in free space(τΛ = 263 ps). However, recent heavy ion collision experiments have observed lifetimes and binding energies of hypernuclei, sparking significant interest.

After 2010, the STAR and ALICE collaborations reported a 20-30% shorter lifetime for 3ΛH. These groups also reported binding energies of BΛ = 406 ± 120(stat.) ± 110(syst.) keV and preliminarily BΛ = 102 ± 63(stat.) ± 67(syst.) keV, respectively. For understanding the correlation between hypertriton's lifetime and binding energy, accurate measurement of these values is crucial.

In October 2022, we conducted decay-pion spectroscopy experiments on s-shell hypernuclei (3ΛH and 4ΛH) at Mainz Microtron (MAMI). Some electro-produced hypernuclei form bound states and decay via two-body weak decay, emitting pions with monochromatic momentum. By measuring this momentum with high-resolution magnetic spectrometers (Δp/p ~ 10-4) and combining it with a Kaon spectrometer to tag strangeness production and suppress background events, we successfully measured the 4ΛH mass with an accuracy of 80 keV in 2014.

In 2022, to enhance the yield of 3ΛH and reduce background events, we changed the target from 9Be to 7Li in this experiment. The 7Li target was positioned at a 90-degree angle to increase luminosity and mitigate the effects of the pion energy struggle. Additionally, we introduced a new technology for beam energy measurement to achieve hypernuclear mass determination with 10-20 keV accuracy.

In this presentation, I will discuss this experimental method and provide an update on the latest analysis.

Presenters

  • Ryoko Kino

    Tohoku University

Authors

  • Ryoko Kino

    Tohoku University

  • Patrick Achenbach

    Jefferson Lab/Jefferson Science Associates, Jefferson Lab

  • Takeru Akiyama

    Tohoku University

  • Ralph Böhm

    FAIR

  • Michael O Distler

    Johannes Gutenberg University Mainz

  • Philipp Eckert

    Johannes Gutenberg University Mainz

  • Anselm Esser

    Johannes Gutenberg University Mainz

  • Julian Geratz

    Johannes Gutenberg University Mainz

  • Christian Helmel

    Johannes Gutenberg University Mainz

  • Matthias Hoek

    Johannes Gutenberg University Mainz

  • Tatsuhiro Ishige

    Tohoku University

  • Kosuke Itabashi

    QUP, WPI research center at KEK

  • Masashi Kaneta

    Tohoku University, Tohoku Univ

  • Pascal Klag

    Johannes Gutenberg University Mainz

  • Harald Merkel

    Johannes Gutenberg University Mainz

  • Masaya Mizuno

    Tohoku University

  • Ulrich Müller

    Johannes Gutenberg University Mainz

  • Sho Nagao

    The University of Tokyo

  • Satoshi N Nakamura

    The University of Tokyo

  • Kotaro Nishi

    The University of Tokyo

  • KAZUKI OKUYAMA

    Tohoku University

  • Josef Pochodzalla

    Johannes Gutenberg University Mainz, Johannes Gutenberg-University Mainz

  • Tianhao Shao

    Johannes Gutenberg University Mainz, Fudan University

  • Björn Sören Schlimme

    Johannes Gutenberg University Mainz

  • Marcell Steinen

    Helmholtz Institute Mainz, GSI Helmholtzzentrum für Schwerionenforschung

  • Koga Tachibana

    Tohoku University

  • Michaela Thiel

    Johannes Gutenberg University Mainz

  • Yuichi Toyama

    Chubu University

  • Keita Uehara

    Tohoku University

  • Daigo Watanabe

    Tohoku University, Tohoku Univ