Plots and Data

We provide data with a consistent choice of units in order to compare in the plots below. Our choice of units:

  • The first column of each csv text file is given as \(\log_{10}(m_N/\mathrm{GeV})\)

  • The second column of each csv text file is given as \(\log_{10}(|U_{\alpha N}|^2)\)

We also give the png, pdf and py plotting code for the figures below.

A bib file containing the references below: References.

Updates

  • 31/03/2023: Added BEBC limits on \(|U_{eN}|^2\) and \(|U_{\tau N}|^2\) from Ref. [173].

Electron Mixing \(|U_{eN}|^2\)

Current Constraints

_images/UeNsq_constraints.png

Fig. 1 Current constraints on the electron neutrino-sterile neutrino mixing \(|U_{eN}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

Daya Bay

[80]

.csv

DANSS

[78]

.csv

KamLAND

[1]

.csv

Solar and KamLAND

[87]

.csv

NEOS

[79]

.csv

SuperKamiokande + IceCube + DeepCore

[87]

.csv

\(^3\mathrm{H}\) Beta Decay (Hiddemann et al.)

[60]

.csv

\(^3\mathrm{H}\) Beta Decay (Mainz)

[61]

.csv

\(^3\mathrm{H}\) Beta Decay (Troitsk 2013)

[62]

.csv

\(^3\mathrm{H}\) Beta Decay (Troitsk 2017)

[63]

.csv

\(^{137}\mathrm{Re}\) Beta Decay

[70]

.csv

\(^{63}\mathrm{Ni}\) Beta Decay

[67]

.csv

\(^{35}\mathrm{S}\) Beta Decay

[65]

.csv

\(^{45}\mathrm{Ca}\) Beta Decay

[66]

.csv

\(^{64}\mathrm{Cu}\) Beta Decay

[68]

.csv

\(^{144}\mathrm{Ce}-^{144}\mathrm{Pr}\) Beta Decay

[69]

.csv

\(^{20}\mathrm{F}\) Beta Decay

[64]

.csv

BeEST \(^{7}\mathrm{Be}\) Beta Decay

[174]

.csv

Rovno

[73]

.csv

Bugey

[74]

.csv

Borexino

[75]

.csv

PIENU

[37]

.csv

Improved Pion Decay Contraints

[38][39]

.csv

PS191 (+ Reanalysis)

[48]

.csv

IHEP-JINR

[49][37]

.csv

NA62

[175]

.csv

T2K

[50]

.csv

SuperKamiokande

[176]

.csv

LNV Meson Decays

[55][3][34][56]

.csv

CHARM

[46][47]

.csv

BEBC

[173]

.csv

BESIII

[57]

.csv

NA3

[45]

.csv

Belle

[44]

.csv

DELPHI

[23]

.csv

L3

[21][22]

.csv

ATLAS Dilepton + Jets

[9]

.csv

ATLAS Trilepton Prompt LNC (LNV)

[7]

.csv (.csv)

CMS Dilepton + Jets

[10]

.csv

CMS Trilepton Prompt LNC (LNV)

[8]

.csv

Higgs Decays

[13]

.csv

Electroweak Precision Data

[91][94][92][95]

.csv

CMB \(\Delta N_{\mathrm{eff}}\)

[137][107]

.csv

CMB + BAO + \(H_0\) (or \(H_0\) Only)

[107]

.csv (.csv)

Sterile Decays before BBN

[101][102]

.csv

NuSTAR X-rays

[115][116]

.csv

Supernovae MSW Effect (Shi and Sigl)

[121]

.csv

Supernovae MSW Effect (Raffelt and Zhou)

[128][177]

.csv

Supernovae MSW Effect (Zhou) Lower (Upper) Limit

[177]

.csv (.csv)

r-process Nucleosynthesis (Nunokawa et al.)

[122]

.csv

Future Sensitivities

_images/UeNsq_future.png

Fig. 2 Future constraints on the electron neutrino-sterile neutrino mixing \(|U_{eN}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

Current LNC Constraints (Blue Shaded)

[A1]

.csv

Current LNV Constraints (Red Shaded)

[A1]

.csv

KATRIN \(^3\mathrm{H}\) \(\beta\) decay

[71]

.csv

TRISTAN \(^3\mathrm{H}\) \(\beta\) decay

[71]

.csv

HUNTER

[178]

.csv, .csv, .csv

BeEST \(^{7}\mathrm{Be}\) Beta Decay

[174]

.csv, .csv, .csv

PIONEER

[179]

.csv

DUNE

[51][52]

.csv (.csv)

DUNE Indirect

[180]

.csv

NA62

[41]

.csv

AL3X

[14]

.csv

FASER-2

[16]

.csv

SHiP

[54]

.csv

MATHUSLA

[17]

.csv

CODEX-b

[181]

.csv

ANUBIS

[182]

.csv

Future LNV Meson Decays

[58]

.csv

LHCb Displaced Vertex

[183][184]

.csv

ATLAS Displaced Vertex

[184]

.csv

CMS Displaced Vertex

[184]

.csv

Lepton Displaced Vertex

[185]

.csv

FCC-ee

[25][186]

.csv

ILC

[26]

.csv

CLIC

[187][28]

.csv (.csv)

LHeC

[27][28][29]

.csv

High Luminosity LHC (and FCC-hh)

[12]

.csv (.csv)

FCC-he

[11][12]

.csv

ATHENA X-rays

[117]

.csv

eROSITA X-rays

[188]

.csv

Muon Mixing \(|U_{\mu N}|^2\)

Current Constraints

_images/UmuNsq_constraints.png

Fig. 3 Current constraints on the muon neutrino-sterile neutrino mixing \(|U_{\mu N}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

IceCUBE

[80]

.csv

MiniBooNE

[78]

.csv

CDHS

[189]

.csv

IceCUBE + DeepCore

[87]

.csv

NOvA

[87]

.csv

SuperKamiokande (Oscillations)

[190]

.csv

MINOS(+)

[191]

.csv

CCFR

[191]

.csv

PSI

[192]

.csv

\(\mu\) Spectrum

[193]

.csv

PIENU

[194]

.csv

KEK

[195][196]

.csv

PS191

[48]

.csv

SuperKamiokande (Decay)

[176]

.csv

E949

[197]

.csv

T2K

[50]

.csv

NA62

[175]

.csv

MicroBooNE

[198][199]

.csv, .csv

LNV Meson Decays

[3][34][55][56]

.csv

NuTeV

[200]

.csv

BEBC

[201]

.csv

FMMF

[202]

.csv

NA3

[45]

.csv

CHARM

[47]

.csv

LHCb

[203]

.csv

Belle

[44]

.csv

L3

[21]

.csv

DELPHI

[23]

.csv

ATLAS

[7]

.csv

CMS

[8]

.csv

Higgs Decays

[13]

.csv

Electroweak Precision Data

[91][94][92][95]

.csv

CMB \(\Delta N_{\mathrm{eff}}\)

[137][107]

.csv

CMB + BAO + \(H_0\) (or \(H_0\) Only)

[107]

.csv (.csv)

Sterile Decays before BBN

[101][102]

.csv

NuSTAR X-rays

[115][116]

.csv

Supernovae MSW Effect (Kopp)

[129]

.csv

Future Sensitivities

_images/UmuNsq_future.png

Fig. 4 Future constraints on the muon neutrino-sterile neutrino mixing \(|U_{\mu N}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

Current LNC Constraints (Blue Shaded)

[A1]

.csv

Current LNV Constraints (Red Shaded)

[A1]

.csv

DUNE

[51][52]

.csv

DUNE Indirect

[180]

.csv

NA62

[41]

.csv

AL3X

[14]

.csv

FASER-2

[16]

.csv

SHiP

[54]

.csv

MATHUSLA

[17]

.csv

CODEX-b

[181]

.csv

ANUBIS

[182]

.csv

Future LNV Meson Decays

[58]

.csv

LHCb Displaced Vertex

[183][184]

.csv

ATLAS Displaced Vertex

[184]

.csv

CMS Displaced Vertex

[184]

.csv

FCC-ee

[25][186]

.csv, .csv

High Luminosity LHC (and FCC-hh)

[12]

.csv (.csv)

ATHENA X-rays

[117]

.csv

eROSITA X-rays

[188]

.csv

Tau Mixing \(|U_{\tau N}|^2\)

Current Constraints

_images/UtauNsq_constraints.png

Fig. 5 Current constraints on the tau neutrino-sterile neutrino mixing \(|U_{\tau N}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

IceCUBE + DeepCore

[204][205]

.csv

SuperKamiokande (Oscillations)

[176]

.csv

T2K (Oscillations)

[176]

.csv

NOvA

[206]

.csv

CHARM

[207][208]

.csv, .csv

BEBC

[173]

.csv

NOMAD

[209]

.csv

Lepton Universality

[210]

.csv

T2K (Decays)

[50]

.csv

SuperKamiokande (Decays)

[176]

.csv

\(B\) Decays

[210]

.csv

L3

[21]

.csv

DELPHI

[23]

.csv

Electroweak Precision Data

[91][94][92][95]

.csv

CMB \(\Delta N_{\mathrm{eff}}\)

[137][107]

.csv

CMB + BAO + \(H_0\) (or \(H_0\) Only)

[107]

.csv (.csv)

Sterile Decays before BBN

[101][102]

.csv

NuSTAR X-rays

[115][116]

.csv

Supernovae MSW Effect (Kopp)

[129]

.csv

Supernovae MSW Effect (Mirizzi)

[211]

.csv

Future Sensitivities

_images/UtauNsq_future.png

Fig. 6 Future constraints on the tau neutrino-sterile neutrino mixing \(|U_{\tau N}|^2\) as a function of the sterile neutrino mass \(m_N\).

Experiment/Analysis

Reference

Data

Current LNC Constraints (Blue Shaded)

[A1]

.csv

DUNE

[51][52]

.csv

NA62

[41]

.csv

FASER-2

[16]

.csv

SHiP

[54]

.csv

MATHUSLA

[17]

.csv

CODEX-b

[181]

.csv

B Factory

[212]

.csv, .csv

Future LNV Meson Decays

[58]

.csv

LHCb Displaced Vertex

[183][184]

.csv

ATLAS Displaced Vertex

[184]

.csv

CMS Displaced Vertex

[184]

.csv

FCC-ee

[25]

.csv

High Luminosity LHC (and FCC-hh)

[12][213]

.csv, .csv (.csv)

ATHENA X-rays

[117]

.csv

eROSITA X-rays

[188]

.csv