2020
DOI: 10.48550/arxiv.2006.08869
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The Light Sgoldstino Phenomenology: Explanations for the Muon $(g-2)$ Deviation and KOTO Anomaly

Xuewen Liu,
Ying Li,
Tianjun Li
et al.

Abstract: In this work, we study the long-standing experimental anomaly in muon (g − 2) and also recent anomalous excess in K L → π 0 + ν ν at the J-PARC KOTO experiment with sgoldstino. After supersymmetry breaking, the interactions between quarks and sgoldstino (s) make the decays K → π + s sizable through loop diagrams, which affects the measurements of decays K → π + invisible. Furthermore, the couplings between photons and sgoldstino contribute to ∆a µ as well as bino-slepton contribution. With satisfying all known… Show more

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Cited by 6 publications
(6 citation statements)
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“…Even though higher-order operators are suppressed when the new physics scale is above the electroweak scale, this is a place where the Standard Model contribution is so suppressed that they can play an important role. In addition, there are models with light new particles (e.g., [45][46][47][48][49][50]). In this case, our classification can be straightforwardly expanded to include new light degrees of freedom in the Hilbert series.…”
Section: Discussionmentioning
confidence: 99%
“…Even though higher-order operators are suppressed when the new physics scale is above the electroweak scale, this is a place where the Standard Model contribution is so suppressed that they can play an important role. In addition, there are models with light new particles (e.g., [45][46][47][48][49][50]). In this case, our classification can be straightforwardly expanded to include new light degrees of freedom in the Hilbert series.…”
Section: Discussionmentioning
confidence: 99%
“…The three-track signature is particularly interesting and is in general always present whenever the five-track process is possible. It also provides a direct test of dark-neutrino explanations to the Mini-BooNE excess [180,181,183,222,223,[261][262][263], where HNLs are produced in muon neutrino interactions inside the detector due to the exchange of a new force. A slice of the dark sector parameter space is shown in Fig.…”
Section: Dark Fermionsmentioning
confidence: 99%
“…( 4), depending on how possible impact of new physics is taken into account [2]. A number of BSM scenarios have been proposed to explain this discrepancy [2,[14][15][16][17][18][19][20][21][22][23][24][25][26][27][28][29][30]. Among them, a prominent role is played by models predicting the existence of a new LLP with the mass m X ∼ 100 MeV, which can be produced in rare kaon decays, K L → π 0 X [2].…”
Section: Koto Experiments and The Anomalymentioning
confidence: 99%