Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 
<b>90</b>
, 062009 (2014)]

Aprile, E.; Agostini, F.; Alfonsi, M.; Arisaka, K.; Arneodo, F.; Auger, M.; Bălan, C.; Barrow, Peter; Baudis, L.; Bauermeister, B.; Behrens, A.; Beltrame, P.; Bokeloh, K.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G. E.; Budnik, R.; Cardoso, J. M. R.; Colijn, A. P.; Contreras, H.; Cussonneau, J. P.; Decowski, M. P.; Duchovni, E.; Fattori, S.; Ferella, A. D.; Fulgione, W.; Gao, F.; Garbini, M.; Geis, C.; Goetzke, L. W.; Grignon, C.; Gross, E.; Hampel, W.; Itay, R.; Kaether, F.; Kessler, G.; Kish, A.; Landsman, H.; Lang, R. F.; Calloch, M. Le; Lellouch, D.; Lévy, C.; Lindemann, Stefan; Lindner, M.; Lopes, J. A. M.; Lung, K.; Lyashenko, A.; MacMullin, S.; Undagoitia, T. Marrodán; Masbou, J.; Massoli, F. V.; Paras, D. Mayani; Fernandez, A. J. Melgarejo; Meng, Y.; Messina, M.; Miguez, B.; Molinario, A.; Murra, M.; Naganoma, J.; Ni, K.; Oberlack, U.; Orrigo, S. E. A.; Pantic, E.; Persiani, R.; Piastra, F.; Pienaar, J.; Plante, G.; Priel, N.; Reichard, S.; Reuter, C.; Rizzo, A.; Rosendahl, S. S.E.; Santos, J. M. F. dos; Sartorelli, G.; Schindler, S. M.; Schreiner, J.; Schümann, M.; Lavina, L. Scotto; Selvi, M.; Shagin, P. M.; Simgen, H.; Teymourian, A.; Thers, D.; Tiseni, A.; Trinchero, G.; Vitells, O.; Wang, H.; Weber, M.; Weinheimer, C.

doi:10.1103/physrevd.95.029904

Cited by 46 publications

(48 citation statements)

References 30 publications

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“…The signal of nonrelativistic χ would be δ-function centered at its mass, CoGeNT [24], EDELWEISS [25], LUX [26], Majorana Demonstrator [27], PANDAX-II [28], XENON100 [29] along with indirect astrophysical bound from solar neutrinos [30] are also shown.…”

Section: Experimental Constraintsmentioning

confidence: 91%

Constraints on bosonic dark matter with low threshold germanium detector at Kuo-Sheng reactor neutrino laboratory

Singh

Ağartıoğlu

et al. 2019

Chinese Journal of Physics

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We report results from searches of pseudoscalar and vector bosonic super-weakly interacting massive particles (super-WIMP) in the TEXONO experiment at the Kuo-Sheng Nuclear Power Station, using 314.15 kg days of data from n-type Point-Contact Germanium detector. The super-WIMPs are absorbed and deposit total energy in the detector, such that the experimental signatures are spectral peaks corresponding to the super-WIMP mass. Measured data are compatible with the background model, and no significant excess of super-WIMP signals are observed. We derived new upper limits on couplings of electrons with the pseudoscalar and vector bosonic super-WIMPs in the sub-keV mass region, assuming they are the dominant contributions to the dark matter density of our galaxy.

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Section: Experimental Constraintsmentioning

confidence: 91%

Constraints on bosonic dark matter with low threshold germanium detector at Kuo-Sheng reactor neutrino laboratory

Singh

Ağartıoğlu

et al. 2019

Chinese Journal of Physics

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“…And the hat Yukawa couplingsŷ e,µ,τ are fixed 8 asŷ e = 0.793152,ŷ µ = 1.137250,ŷ τ = 0.968747 by using the numerical values of Eq. (35) in quark sector via the empirical results m e = 0.511 MeV, m µ = 105.683 MeV, and m τ = 1776.86 MeV [29].…”

Section: Charged-leptons and Flavored-axionsmentioning

confidence: 99%

Compact model for quarks and leptons via flavored axions

Ahn

2018

Phys. Rev. D

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We show how the scales responsible for Peccei-Quinn (PQ), seesaw, and Froggatt and Nielsen (FN) mechanisms can be fixed, by constructing a compact model for resolving rather recent, but fast-growing issues in astro-particle physics, including quark and leptonic mixings and CP violations, high-energy neutrinos, QCD axion, and axion cooling of stars. The model is motivated by the flavored PQ symmetry for unifying the flavor physics and string theory. The QCD axion decay constant congruent to the seesaw scale, through its connection to the astro-particle constraints of both the stellar evolution induced by the flavored-axion bremsstrahlung off electrons e + Ze → Ze + e + A i and the rare flavor-changing decay process induced by the flavored-axion−0.84 × 10 10 GeV (consequently, the QCD axion mass m a = 1.54 +0.48 −0.29 × 10 −4 eV, Compton wavelength of its oscillation λ a = 8.04 +1.90 −1.90 mm, and axion to neutron coupling g Ann = 2.14 +0.66 −0.41 × 10 −12 , etc.). Subsequently, the scale associated to FN mechanism is dynamically fixed, Λ = 2.04 +0.48 −0.48 × 10 11 GeV, through its connection to the standard model fermion masses and mixings, and such fundamental scale might give a hint where some string moduli are stabilized in type-IIB string vacua. In the near future, the NA62 experiment expected to reach the sensitivity of Br(K + → π + + A i ) < 1.0 × 10 −12 will probe the flavored-axions or exclude the model, if the astrophysical constraint of star cooling is really responsible for the flavored-axion. PACS numbers: * Here 'compact' model means a model that provides only requisite parameters it is easy to disprove. † Electronic address: axionahn@naver.com 1 See, most recent its related simple toy models ((non-)supersymmetric versions) in Ref . [5], see also Ref. [6]. 2 On this issue we will consider flavored-axion [8] as a cold dark matter in the next project. The scale in Eq. (44) we found is available for explaining dark matter, and finding it in experiments can change the fundamental understanding of the universe.

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“…Several experiments have reported the corresponding results [8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23] using the mechanism arising from the couplings to electrons:…”

Section: Introductionmentioning

confidence: 99%

Improved limits on solar axions and bosonic dark matter from the CDEX-1B experiment using the profile likelihood ratio method

Wang¹,

Yue²,

Liu³

et al. 2020

Phys. Rev. D

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We present improved constraints on couplings of solar axions and more generic bosonic dark matter particles using 737.1 kg-days of data from the CDEX-1B experiment. The CDEX-1B experiment, located at the China Jinping Underground Laboratory, primarily aims at the direct detection of WIMPs using a p-type point-contact germanium detector. We develop the profile likelihood ratio method for analysis of data in the presence of backgrounds. The background modeling is compatible with the data and no excess signals are observed. An energy threshold of 160 eV was achieved. This significantly improve the sensitivity for the bosonic dark matter below 0.8 keV. Limits are also placed on the coupling gAe < 2.26 × 10 −11 from Compton, bremsstrahlung, atomic-recombination and deexcitation channels and g ef f AN × gAe < 4.14 × 10 −17 from a 57 Fe M1 transition at 90% confidence level. All the constrains improve over our previous results.

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Erratum: First axion results from the XENON100 experiment [Phys. Rev. D 90 , 062009 (2014)]

Cited by 46 publications

References 30 publications

Constraints on bosonic dark matter with low threshold germanium detector at Kuo-Sheng reactor neutrino laboratory

Constraints on bosonic dark matter with low threshold germanium detector at Kuo-Sheng reactor neutrino laboratory

Compact model for quarks and leptons via flavored axions

Improved limits on solar axions and bosonic dark matter from the CDEX-1B experiment using the profile likelihood ratio method

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