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Journal articles on the topic 'Rich light'

Author: Grafiati
Published: 4 June 2021
Last updated: 10 February 2022

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1

Bang, J. M., F. A. Gareev, G. S. Kazacha, and A. M. Kalinin. "Neutron-rich light nuclei." Physica Scripta 41, no. 2 (February 1, 1990): 202–6. http://dx.doi.org/10.1088/0031-8949/41/2/003.

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2

Jelavić Malenica, D., M. Milin, A. Di Pietro, P. Figuera, M. Lattuada, D. Miljanić, A. Musumarra, et al. "Clusters in neutron-rich light nuclei." EPJ Web of Conferences 117 (2016): 07007. http://dx.doi.org/10.1051/epjconf/201611707007.

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3

Broemmelsiek, Daniel R. "HERA-B RICH light collection system." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 433, no. 1-2 (August 1999): 136–42. http://dx.doi.org/10.1016/s0168-9002(99)00294-6.

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4

Williams, Peter J. "Rich prospects for light-wave ICs." Physics World 4, no. 9 (September 1991): 63–65. http://dx.doi.org/10.1088/2058-7058/4/9/32.

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5

Torilov, S. Yu, K. A. Gridnev, and T. V. Korovitskaya. "Rotational bands in light neutron-rich nuclei." Bulletin of the Russian Academy of Sciences: Physics 76, no. 8 (August 2012): 854–56. http://dx.doi.org/10.3103/s1062873812080278.

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6

Sagawa, Hiroyuki, and C. A. Bertulani. "Multipole Excitations in Light Neutron-Rich Nuclei." Progress of Theoretical Physics Supplement 124 (1996): 143–53. http://dx.doi.org/10.1143/ptps.124.143.

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7

Whitelock, Patricia. "Infrared Light Curves of Carbon-Rich Variables." Symposium - International Astronomical Union 177 (2000): 179–90. http://dx.doi.org/10.1017/s0074180900002394.

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Long-term trends in the infrared (JHKL) light curves of various carbon variables are described. Some stars, e.g. the semi-regular variables R Scl and GM CMa, show multiple periodicities; others, particularly the Miras with moderately thick dust-shells, show more erratic long-term changes. The light curves for R For, which have been intensively monitored over 20 years, show a pattern which is reminiscent of that seen for R CrB stars. This pattern is superimposed on regular large-amplitude Mira pulsations. The multi-periodic and erratic behaviour of these stars is compared with the predictions from various models.
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8

Kanada-En'yo, Y., Y. Taniguchi, and M. Kimura. "Cluster structure in light neutron-rich nuclei." Journal of Physics: Conference Series 111 (May 1, 2008): 012002. http://dx.doi.org/10.1088/1742-6596/111/1/012002.

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9

Bohlen, H. G., W. von Oertzen, R. Kalpakchieva, T. N. Massey, T. Dorsch, M. Milin, C. Schulz, T. Kokalova, and C. Wheldon. "Band structures in light neutron-rich nuclei." Journal of Physics: Conference Series 111 (May 1, 2008): 012021. http://dx.doi.org/10.1088/1742-6596/111/1/012021.

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10

Korsheninnikov, A. A., D. V. Aleksandrov, N. Aoi, Y. Doki, N. Inabe, M. Fujimaki, T. Kobayashi, et al. "Experimental studies of light neutron rich nuclei." Nuclear Physics A 588, no. 1 (May 1995): c23—c28. http://dx.doi.org/10.1016/0375-9474(95)00094-h.

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11

Ishihara, M. "Current topics on light neutron-rich nuclei." Nuclear Physics A 588, no. 1 (May 1995): c49—c58. http://dx.doi.org/10.1016/0375-9474(95)00098-l.

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12

He, Chao, Hui Hua, Xiangqing Li, and Bo Wang. "β-Decay of Light Neutron-Rich Nuclei." Plasma Science and Technology 14, no. 7 (July 2012): 610–13. http://dx.doi.org/10.1088/1009-0630/14/7/10.

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13

Dal Negro, L., J. H. Yi, L. C. Kimerling, S. Hamel, A. Williamson, and G. Galli. "Light emission from silicon-rich nitride nanostructures." Applied Physics Letters 88, no. 18 (May 2006): 183103. http://dx.doi.org/10.1063/1.2191956.

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14

Curtin, M. S., L. H. Harwood, J. A. Nolen, B. Sherrill, Z. Q. Xie, and B. A. Brown. "Lifetime measurements of neutron-rich light isotopesBe14andC17." Physical Review Letters 56, no. 1 (January 6, 1986): 34–37. http://dx.doi.org/10.1103/physrevlett.56.34.

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15

Hoshino, T., H. Sagawa, and A. Arima. "Giant resonances of light neutron-rich nuclei." Nuclear Physics A 523, no. 2 (February 1991): 228–46. http://dx.doi.org/10.1016/0375-9474(91)90002-n.

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16

Huang Rui, Dong Heng-Ping, Wang Dan-Qing, Chen Kun-Ji, Ding Hong-Lin, Xu Jun, Li Wei, and Ma Zhong-Yuan. "Electroluminescence from Si-rich SiNx/N-rich SiNy multilayer light-emitting devices." Acta Physica Sinica 58, no. 3 (2009): 2072. http://dx.doi.org/10.7498/aps.58.2072.

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17

D'Ambrosio, C. "The future of RICH detectors through the light of the LHCb RICH." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 876 (December 2017): 194–97. http://dx.doi.org/10.1016/j.nima.2017.02.076.

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18

Khomenkova, L., O. Kolomys, M. Baran, A. Kuchuk, V. Strelchuk, Ye Venger, V. Kladko, J. Jedrzejewski, I. Balberg, and N. Korsunska. "Structure and light emission of Si-rich Al2O3 and Si-rich-SiO2 nanocomposites." Microelectronic Engineering 125 (August 2014): 62–67. http://dx.doi.org/10.1016/j.mee.2013.12.001.

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19

Dias, L., C. Coelho, Bruno Trindade, and F. H. Froes. "Mg-Rich Light Alloys Synthesised by Mechanical Alloying." Key Engineering Materials 230-232 (October 2002): 283–86. http://dx.doi.org/10.4028/www.scientific.net/kem.230-232.283.

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20

Cortina-Gil, M. D., P. Roussel-Chomaz, N. Alamanos, J. Barrette, W. Mittig, F. S. Dietrich, F. Auger, et al. "Proton elastic scattering on light neutron-rich nuclei." Physics Letters B 401, no. 1-2 (May 1997): 9–14. http://dx.doi.org/10.1016/s0370-2693(97)00321-3.

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21

Orr, N. A. "Haloes and clustering in light, neutron-rich nuclei." European Physical Journal A 15, no. 1-2 (September 2002): 109–13. http://dx.doi.org/10.1140/epja/i2001-10236-6.

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22

Cortina-Gil, M. D., A. Pakou, N. Alamanos, W. Mittig, P. Roussel-Chomaz, F. Auger, J. Barrette, et al. "Charge-exchange reaction with light neutron-rich beams." Journal of Physics G: Nuclear and Particle Physics 24, no. 8 (August 1, 1998): 1547–52. http://dx.doi.org/10.1088/0954-3899/24/8/032.

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23

Itagaki, Naoyuki, Shigeto Okabe, and Kiyomi Ikeda. "Molecular-Orbital Structure in Light Neutron-Rich Nuclei." Progress of Theoretical Physics Supplement 142 (2001): 297–323. http://dx.doi.org/10.1143/ptps.142.297.

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24

HAGINO, K., H. SAGAWA, and P. SCHUCK. "DI-NEUTRON CORRELATION IN LIGHT NEUTRON-RICH NUCLEI." International Journal of Modern Physics E 18, no. 10 (November 2009): 2045–49. http://dx.doi.org/10.1142/s0218301309014263.

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Using a three-body model with density-dependent contact interaction, we discuss the root mean square distance between the two valence neutrons in 11 Li nuclues as a function of the center of mass of the neutrons relative to the core nucleus 9 Li . We show that the mean distance takes a pronounced minimum around the surface of the nucleus, indicating a strong surface di-neutron correlation. We demonstrate that the pairing correlation plays an essential role in this behavior. We also discuss the di-neutron structure in the 8 He nucleus.
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25

Nappi, E. "RICH detectors operated in the visible light region." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 409, no. 1-3 (May 1998): 417–22. http://dx.doi.org/10.1016/s0168-9002(98)00116-8.

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26

Itagaki, N., K. Hagino, T. Otsuka, S. Okabe, and K. Ikeda. "Importance of clustering in light neutron-rich nuclei." Nuclear Physics A 719 (May 2003): C205—C208. http://dx.doi.org/10.1016/s0375-9474(03)00918-7.

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27

Le´pine-Szily, A., J. M. Oliveira, D. Galante, G. Amadio, R. Lichtentha¨ler, H. G. Bohlen, A. N. Ostrowski, et al. "Spectroscopy of light proton-rich nuclei:9C and15F." Nuclear Physics A 734 (April 2004): 331–36. http://dx.doi.org/10.1016/j.nuclphysa.2004.01.060.

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28

Itagaki, N., S. Aoyama, T. Otsuka, T. Yoshida, S. Okabe, and K. Ikeda. "Exotic cluster structure in light neutron-rich nuclei." Nuclear Physics A 738 (June 2004): 17–23. http://dx.doi.org/10.1016/j.nuclphysa.2004.04.006.

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29

Lupi, Federico Ferrarese, Daniel Navarro-Urrios, Josep Monserrat, Carlos Dominguez, Paolo Pellegrino, and Blas Garrido. "High Q light-emitting Si-rich Si_3N_4 microdisks." Optics Letters 36, no. 8 (April 6, 2011): 1344. http://dx.doi.org/10.1364/ol.36.001344.

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30

Itagaki, N., T. Otsuka, S. Okabe, and al et. "Exotic Cluster Structure in Light Neutron-Rich Nuclei." Acta Physica Hungarica A) Heavy Ion Physics 18, no. 2-4 (November 1, 2003): 173–78. http://dx.doi.org/10.1556/aph.18.2003.2-4.9.

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31

ZHANG, H. Y., W. Q. SHEN, Y. G. MA, X. Z. CAI, D. Q. FANG, C. ZHONG, Y. B. WEI, et al. "POSSIBLE EXOTIC STRUCTURE IN LIGHT PROTON-RICH NUCLEI." Modern Physics Letters A 18, no. 02n06 (February 28, 2003): 151–61. http://dx.doi.org/10.1142/s0217732303010156.

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Radioactive ion beams were produced through the projectile fragmentation induced by 69MeV/nucleon 36 Ar primary beam on a 9 Be target. Measurements of reaction cross section (σR) for some proton-rich nuclei on carbon target at intermediate energies around 30MeV/nucleon have been performed on RIBLL of HIRFL by transmission method and transmission plus transportation method. The experimental σR values for 23Al and 27P are abnormally large compared with their neighboring nuclei and that of 17F has an enhancement compared with the neighboring isotopes. It suggests anomalously large matter root-mean-square radii and proton halo structure in 23 Al and 27 P . The experimental σR values and momentum distribution of fragmentation reaction product for 31 Cl , 32 Cl , 33 Cl , 28 S , 29 S were performed also on RIBLL by transmission and transportation method. These data are in analyzing. The calculation of relativistic density-dependent Hartree shows that the nuclei 23 Al , 27 P , 31 Cl may have proton-halo structure and 17F, 32Cl may have proton-skin structure. New experiment on the search for new nuclides 25 P and 26 S in proton drip line is also described. The significance of these measurements and possible proton halo and skin for light proton-rich nuclei has been discussed.
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32

Gillibert, A., L. Bianchi, A. Cunsolo, B. Fernandez, A. Foti, J. Gastebois, Ch Gregoire, et al. "Mass measurement of light neutron-rich fragmentation products." Physics Letters B 176, no. 3-4 (August 1986): 317–21. http://dx.doi.org/10.1016/0370-2693(86)90171-1.

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33

Sagawa, H., and H. Toki. "Hartree-Fock calculations of light neutron-rich nuclei." Journal of Physics G: Nuclear Physics 13, no. 4 (April 1987): 453–61. http://dx.doi.org/10.1088/0305-4616/13/4/008.

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34

Padilla, S., G. Orive, and E. Anitua. "Shedding light on biosafety of platelet rich plasma." Expert Opinion on Biological Therapy 17, no. 8 (July 6, 2017): 1047–48. http://dx.doi.org/10.1080/14712598.2017.1349487.

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35

Hoshino, T., H. Sagawa, and A. Arima. "Shell-model study of light neutron-rich nuclei." Nuclear Physics A 506, no. 2 (January 1990): 271–92. http://dx.doi.org/10.1016/0375-9474(90)90387-2.

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36

Sahu, S., M. Ghosh, and D. K. Bhattacharyya. "Utilization of unsaponifiable matter from rice bran oil fatty acid distillate for preparing an antioxidant-rich oleogel and evaluation of its properties." Grasas y Aceites 71, no. 1 (January 14, 2020): 336. http://dx.doi.org/10.3989/gya.0938182.

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Rice bran oil fatty acid distillate (RBOFAD) is an important by-product obtained from the physical refining process. This fatty acid distillate contains high a amount of Unsaponifiable Matter (γ-oryzanol 3.27 gm/100gm UM; total tocopherol 10.93 mg/100 g UM; total phytosterol 21.81 g/100g UM; squalene 1.15 g/100 g UM and total fatty alcohol 73.34 g/100 g UM) and free fatty acids. Antioxidant-rich Oleogels were obtained from rice bran wax (RBW), rice bran oil fatty acid distillate (RBOFAD) and refined rice bran oil. The main objective of this study was to utilize the antioxidant-rich unsaponifiable matter of RBOFAD (UMRBOFAD) as an organogelator along with rice bran wax, which also acts as a good organogelator. Antioxidant-rich oleogel was prepared using UMRBFAD, ethylcellulose (EC) and RBW at 2%, 2%, 3% on weight basis, respectively, in refined rice bran oil and this antioxidant-rich oleogel was compared with rice bran oil oleogel using RBW at 7% on weight basis of rice bran oil. These oleogels were evaluated using a combination of techniques such as differential scanning calorimetry (DSC), polarized light microscopy (PLM), Viscosity, synchrotron radiation X-ray diffraction (SR-XRD) and FTIR Spectroscopy. The differential scanning calorimetry (DSC) measured the thermal properties of rice bran oil oleogel and high antioxidant-rich oleogel. Polarized light microscopy images revealed needle-like crystals for RBW. SR-XRD measurements were used for clarification of the crystal structures of the building blocks of these oleogels. The antioxidant activities of oleogels were evaluated involving DPPH and ABTS assays.
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37

Li, J., O. H. Y. Zalloum, T. Roschuk, C. L. Heng, J. Wojcik, and P. Mascher. "Light Emission from Rare-Earth Doped Silicon Nanostructures." Advances in Optical Technologies 2008 (May 13, 2008): 1–10. http://dx.doi.org/10.1155/2008/295601.

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Rare earth (Tb or Ce)-doped silicon oxides were deposited by electron cyclotron resonance plasma-enhanced chemical vapour deposition (ECR-PECVD). Silicon nanocrystals (Si-ncs) were formed in the silicon-rich films during certain annealing processes. Photoluminescence (PL) properties of the films were found to be highly dependent on the deposition parameters and annealing conditions. We propose that the presence of a novel sensitizer in the Tb-doped oxygen-rich films is responsible for the indirect excitation of the Tb emission, while in the Tb-doped silicon-rich films the Tb emission is excited by the Si-ncs through an exciton-mediated energy transfer. In the Ce-doped oxygen-rich films, an abrupt increase of the Ce emission intensity was observed after annealing at 1200∘C. This effect is tentatively attributed to the formation of Ce silicate. In the Ce-doped silicon-rich films, the Ce emission was absent at annealing temperatures lower than 1100∘C due to the strong absorption of Si-ncs. Optimal film compositions and annealing conditions for maximizing the PL intensities of the rare earths in the films have been determined. The light emissions from these films were very bright and can be easily observed even under room lighting conditions.
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38

Chen, Haihang, and Yiming Xu. "Photocatalytic organic degradation over W-rich and Cu-rich CuWO4 under UV and visible light." RSC Advances 5, no. 11 (2015): 8108–13. http://dx.doi.org/10.1039/c4ra13952f.

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39

Weiss, Peter. "Light Goes on for Antimatter-Rich H 2 O." Science News 154, no. 24 (December 12, 1998): 375. http://dx.doi.org/10.2307/4011019.

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40

Metlica, F. C. D. "Development of light-weight spherical mirrors for RICH detectors." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 595, no. 1 (September 2008): 197–99. http://dx.doi.org/10.1016/j.nima.2008.07.026.

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41

Ren, Z., B. Chen, Z. Ma, and W. Mittig. "Relativistic mean-field study of light neutron-rich nuclei." Journal of Physics G: Nuclear and Particle Physics 21, no. 9 (September 1, 1995): 1269–72. http://dx.doi.org/10.1088/0954-3899/21/9/012.

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42

Kalpakchieva, R. "Very neutron-rich isotopes of light elements: Nuclear structure." Physics of Particles and Nuclei 30, no. 6 (November 1999): 627. http://dx.doi.org/10.1134/1.953122.

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43

Nagarajan, S., Y. S. Lee, M. Senthil Kumar, O. H. Cha, C.-H. Hong, and E.-K. Suh. "White light generation from In-rich InAlGaN/InGaN heterostructures." Journal of Physics D: Applied Physics 41, no. 1 (December 12, 2007): 012001. http://dx.doi.org/10.1088/0022-3727/41/1/012001.

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44

Singh, P., R. Kumar, and R. Kharab. "Coulomb breakup of neutron-rich isotopes of light nuclei." Physics of Atomic Nuclei 71, no. 11 (November 2008): 1932–39. http://dx.doi.org/10.1134/s1063778808110100.

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45

Gornov, M. G., Yu B. Gurov, P. V. Morokhov, S. V. Lapushkin, V. A. Pechkurov, B. A. Chernyshev, V. G. Sandukovsky, and E. A. Pasyuk. "Multilayer semiconductor spectrometer for studying light neutron-rich nuclei." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 446, no. 3 (May 2000): 461–68. http://dx.doi.org/10.1016/s0168-9002(99)00921-3.

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46

Penionzhkevich, Yu E., R. Kalpakchieva, and S. M. Lukyanov. "Particle stability of very neutron-rich very light nuclei." Nuclear Physics A 722 (July 2003): C170—C175. http://dx.doi.org/10.1016/s0375-9474(03)01354-x.

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47

Lépine-Szily, A., J. M. Oliveira, D. Galante, G. Amadio, V. Vanin, R. Lichtenthäler, V. Guimarães, et al. "Spectroscopy of light proton-rich unbound nuclei: 15F, 10,11N." Nuclear Physics A 722 (July 2003): C512—C517. http://dx.doi.org/10.1016/s0375-9474(03)01418-0.

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48

Zhang, H. Y., W. Q. Shen, Z. Z. Ren, Y. G. Ma, J. G. Chen, X. Z. Cai, C. Zhong, et al. "Investigations on light proton-rich nuclei with exotic structure." Nuclear Physics A 722 (July 2003): C518—C522. http://dx.doi.org/10.1016/s0375-9474(03)01419-2.

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49

Lin, Zewen, Rui Huang, Yanqing Guo, Chao Song, Zhenxu Lin, Yi Zhang, Xiang Wang, Jie Song, Hongliang Li, and Xintang Huang. "Near-infrared light emission from Si-rich oxynitride nanostructures." Optical Materials Express 4, no. 4 (March 26, 2014): 816. http://dx.doi.org/10.1364/ome.4.000816.

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50

Spencer, L. "'That Light of Outrage' : The Historicism of Adrienne Rich." English 51, no. 200 (June 1, 2002): 145–60. http://dx.doi.org/10.1093/english/51.200.145.

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