Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Sharma, M. K."'
Publikováno v:
Phys. Rev. D 108, 083003 (2023)
Over the past two decades, significant strides have been made in the study of Dark Matter (DM) admixed neutron stars and their associated properties. However, an intriguing facet regarding the effect of DM on magnetized neutron stars still remains un
Externí odkaz:
http://arxiv.org/abs/2306.17510
Autor:
Auty, D. J., Bartlett, D., Biller, S. D., Chauhan, D., Chen, M., Chkvorets, O., Connolly, S., Dai, X., Fletcher, E., Frankiewicz, K., Gooding, D., Grant, C., Hall, S., Horne, D., Hans, S., Hreljac, B., Kaptanoglu, T., Krar, B., Kraus, C., Kroupova', T., Lam, I., Liu, Y., Maguire, S., Miller, C., Manecki, S., Rosero, R., Segui, L., Sharma, M. K., Tacchino, S., Tam, B., Tian, L., Veinot, J. G. C., Walton, S. C., Weigand, J. J., Wright, A., Yeh, M., Zhao, T.
Publikováno v:
Nuclear Inst. and Methods in Physics Research, A 1051 (2023) 168204
A method has been developed to load tellurium into liquid scintillator so as to permit searches for neutrinoless double beta decay with high sensitivity. The approach involves the synthesis of an oil-soluble tellurium compound from telluric acid and
Externí odkaz:
http://arxiv.org/abs/2212.12444
Publikováno v:
Phys. Rev. D 107, 043022 (2023)
Even though the crystallize nature of the neutron star crust plays a pivotal role in describing various fascinating astrophysical observations, its microscopic structure is not fully understood in the presence of a colossal magnetic field. In the pre
Externí odkaz:
http://arxiv.org/abs/2211.07339
Publikováno v:
Phys. Rev. D 106, 023031 (2022)
We study the properties of pasta structures and their influence on the neutron star observables employing the effective relativistic mean-field (E-RMF) model. The compressible liquid drop model is used to incorporate the finite size effects, consider
Externí odkaz:
http://arxiv.org/abs/2203.16827
Publikováno v:
Phys. Rev. D 105, 043017 (2022)
We use the effective relativistic mean-field (E-RMF) model to study the crustal properties of the neutron star. The unified equations of state (EoS) are constructed using recently developed E-RMF parameter sets, such as FSUGarnet, IOPB-I, and G3. The
Externí odkaz:
http://arxiv.org/abs/2111.07278
Autor:
Collaboration, SNO, Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Barão, F., Barros, N., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Boulay, M., Caden, E., Callaghan, E. J., Caravaca, J., Chen, M., Chkvorets, O., Cleveland, B., Cookman, D., Corning, J., Cox, M. A., Deluce, C., Depatie, M. M., Di Lodovico, F., Dittmer, J., Falk, E., Fatemighomi, N., Fischer, V., Ford, R., Frankiewicz, K., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hartnell, J., Heintzelman, W. J., Helmer, R. L., Hu, J., Hunt-Stokes, R., Hussain, S. M. A., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Khan, H., Klein, J. R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Lam, I., Land, B. J., LaTorre, A., Lawson, I., Lebanowski, L., Lefebvre, C., Li, A., Lidgard, J., Lin, Y. H., Liu, Y., Lozza, V., Luo, M., Maio, A., Manecki, S., Maneira, J., Martin, R. D., McCauley, N., McDonald, A. B., Meyer, M., Mills, C., Morton-Blake, I., Nae, S., Nirkko, M., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Page, J., Parker, W., Paton, J., Peeters, S. J. M., Pershing, T., Pickard, L., Prior, G., Ravi, P., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rumleskie, J., Semenec, I., Shaker, F., Sharma, M. K., Skensved, P., Smiley, M., Stainforth, R., Svoboda, R., Tam, B., Tseng, J., Turner, E., Valder, S., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., Wang, J., Ward, M., Weigand, J. J., Wilson, J. R., Wright, A., Yanez, J. P., Yeh, M., Yu, S., Zhang, T., Zhang, Y., Zuber, K., Zummo, A.
Publikováno v:
JINST 16 (2021) P10021
SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector acquired data for two years as a pure w
Externí odkaz:
http://arxiv.org/abs/2106.03951
Autor:
Collaboration, SNO, Albanese, V., Alves, R., Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Back, S., Barão, F., Barnard, Z., Barr, A., Barros, N., Bartlett, D., Bayes, R., Beaudoin, C., Beier, E. W., Berardi, G., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Connors, C., Cookman, D., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Di Lodovico, F., Dittmer, J., Doxtator, A., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Felber, C., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gauthier, J., Gibson-Foster, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Hodak, B., Hodak, M., Hood, M., Horne, D., Hreljac, B., Hu, J., Hussain, S. M. A., Iida, T., Inácio, A. S., Jackson, C. M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupová, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., Larochelle, P., Larose, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Li, O., Lidgard, J., Liggins, B., Liimatainen, P., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mathewson, A., McCauley, N., McDonald, A. B., McFarlane, K., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morissette, B., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Read, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Ritchie, I., Robertson, A., Robertson, B. C., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Sörensen, A., St-Amant, M., Stainforth, R., Stankiewicz, S., Strait, M., Stringer, M. I., Stripay, A., Svoboda, R., Tacchino, S., Tam, B., Tanguay, C., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Vázquez-Jáuregui, E., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Walker, J. M. G., Walker, M., Wallig, J., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., Zummo, A.
Publikováno v:
The SNO+ collaboration, 2021 JINST 16 P08059
The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta ($0\nu\beta\beta$) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural te
Externí odkaz:
http://arxiv.org/abs/2104.11687
Autor:
Collaboration, SNO, Anderson, M. R., Andringa, S., Anselmo, L., Arushanova, E., Asahi, S., Askins, M., Auty, D. J., Back, A. R., Barnard, Z., Barros, N., Bartlett, D., Barão, F., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Braid, D., Caden, E., Callaghan, E. J., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chen, M., Chkvorets, O., Clark, K. J., Cleveland, B., Cookman, D., Connors, C., Coulter, I. T., Cox, M. A., Cressy, D., Dai, X., Darrach, C., Davis-Purcell, B., Deluce, C., Depatie, M. M., Descamps, F., Dittmer, J., Di Lodovico, F., Duhaime, N., Duncan, F., Dunger, J., Earle, A. D., Fabris, D., Falk, E., Farrugia, A., Fatemighomi, N., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gagnon, N., Gaur, A., Gilje, K., González-Reina, O. I., Gooding, D., Gorel, P., Graham, K., Grant, C., Grove, J., Grullon, S., Guillian, E., Hall, S., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Heise, J., Helmer, R. L., Horne, D., Hreljac, B., Hu, J., Hussain, A. S. M., Iida, T., Inácio, A. S., Jackson, M., Jelley, N. A., Jillings, C. J., Jones, C., Jones, P. G., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keeter, K., Kefelian, C., Khaghani, P., Kippenbrock, L., Klein, J. R., Knapik, R., Kofron, J., Kormos, L. L., Korte, S., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Labe, K., Lafleur, F., Lam, I., Lan, C., Land, B. J., Lane, R., Langrock, S., LaTorre, A., Lawson, I., Lebanowski, L., Lefeuvre, G. M., Leming, E. J., Li, A., Lidgard, J., Liggins, B., Lin, Y. H., Liu, X., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Majumdar, K., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., Mauel, J., McCauley, N., McDonald, A. B., Mekarski, P., Meyer, M., Miller, C., Mills, C., Mlejnek, M., Mony, E., Morton-Blake, I., Mottram, M. J., Nae, S., Nirkko, M., Nolan, L. J., Novikov, V. M., O'Keeffe, H. M., O'Sullivan, E., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Petriw, Z., Petzoldt, J., Pickard, L., Pracsovics, D., Prior, G., Prouty, J. C., Quirk, S., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Robertson, A., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Schumaker, M. A., Schwendener, M. H., Scislowski, D., Secrest, J., Seddighin, M., Segui, L., Seibert, S., Semenec, I., Shaker, F., Shantz, T., Sharma, M. K., Shokair, T. M., Sibley, L., Sinclair, J. R., Singh, K., Skensved, P., Smiley, M., Sonley, T., Stainforth, R., Strait, M., Stringer, M. I., Svoboda, R., Sörensen, A., Tam, B., Tatar, J., Tian, L., Tolich, N., Tseng, J., Tseung, H. W. C., Turner, E., Van Berg, R., Veinot, J. G. C., Virtue, C. J., von Krosigk, B., Vázquez-Jáuregui, E., Walker, J. M. G., Walker, M., Walton, S. C., Wang, J., Ward, M., Wasalski, O., Waterfield, J., Weigand, J. J., White, R. F., Wilson, J. R., Winchester, T. J., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zhao, T., Zuber, K., Zummo, A.
Publikováno v:
JINST 16 (2021) P05009
A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-exist
Externí odkaz:
http://arxiv.org/abs/2011.12924
Autor:
Collaboration, The SNO, Anderson, M. R., Andringa, S., Askins, M., Auty, D. J., Barros, N., Barão, F., Bayes, R., Beier, E. W., Bialek, A., Biller, S. D., Blucher, E., Bonventre, R., Boulay, M., Caden, E., Callaghan, E. J., Caravaca, J., Chauhan, D., Chen, M., Chkvorets, O., Cleveland, B., Cox, M. A., Depatie, M. M., Dittmer, J., Di Lodovico, F., Earle, A. D., Falk, E., Fatemighomi, N., Fischer, V., Fletcher, E., Ford, R., Frankiewicz, K., Gilje, K., Gooding, D., Grant, C., Grove, J., Hallin, A. L., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Heintzelman, W. J., Helmer, R. L., Horne, D., Hreljac, B., Hu, J., Hussain, A. S. M., Inácio, A. S., Jillings, C. J., Kaptanoglu, T., Khaghani, P., Klein, J. R., Knapik, R., Kormos, L. L., Krar, B., Kraus, C., Krauss, C. B., Kroupova, T., Lam, I., Land, B. J., LaTorre, A., Lawson, I., Lebanowski, L., Leming, E. J., Li, A., Lidgard, J., Liggins, B., Lin, Y. H., Liu, Y., Lozza, V., Luo, M., Maguire, S., Maio, A., Manecki, S., Maneira, J., Martin, R. D., Marzec, E., Mastbaum, A., McCauley, N., McDonald, A. B., Mekarski, P., Meyer, M., Mills, C., Morton-Blake, I., Nae, S., Nirkko, M., Nolan, L. J., O'Keeffe, H. M., Gann, G. D. Orebi, Parnell, M. J., Paton, J., Peeters, S. J. M., Pershing, T., Pickard, L., Prior, G., Reichold, A., Riccetto, S., Richardson, R., Rigan, M., Rose, J., Rosero, R., Rost, P. M., Rumleskie, J., Semenec, I., Shaker, F., Sharma, M. K., Singh, K., Skensved, P., Smiley, M., Stringer, M. I., Svoboda, R., Tam, B., Tian, L., Tseng, J., Turner, E., Van Berg, R., Veinot, J. G. C., Virtue, C. J., Vázquez-Jáuregui, E., Walton, S. C., Wang, J., Ward, M., Weigand, J. J., Wilson, J. R., Woosaree, P., Wright, A., Yanez, J. P., Yeh, M., Zhang, T., Zhang, Y., Zuber, K., Zummo, A.
Publikováno v:
Phys. Rev. C 102, 014002 (2020)
The SNO+ experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV $\gamma$ produced by neutron capture on hydrogen have been made using an Am-Be calibration source, for which
Externí odkaz:
http://arxiv.org/abs/2002.10351
Autor:
STAR Collaboration, Adamczyk, L., Adkins, J. K., Agakishiev, G., Aggarwal, M. M., Ahammed, Z., Ajitanand, N. N., Alekseev, I., Anderson, D. M., Aoyama, R., Aparin, A., Arkhipkin, D., Aschenauer, E. C., Ashraf, M. U., Attri, A., Averichev, G. S., Bai, X., Bairathi, V., Behera, A., Bellwied, R., Bhasin, A., Bhati, A. K., Bhattarai, P., Bielcik, J., Bielcikova, J., Bland, L. C., Bordyuzhin, I. G., Bouchet, J., Brandenburg, J. D., Brandin, A. V., Brown, D., Bunzarov, I., Butterworth, J., Caines, H., Sánchez, M. Calderón de la Barca, Campbell, J. M., Cebra, D., Chakaberia, I., Chaloupka, P., Chang, Z., Chankova-Bunzarova, N., Chatterjee, A., Chattopadhyay, S., Chen, X., Chen, J. H., Cheng, J., Cherney, M., Christie, W., Contin, G., Crawford, H. J., Das, S., De Silva, L. C., Debbe, R. R., Dedovich, T. G., Deng, J., Derevschikov, A. A., Didenko, L., Dilks, C., Dong, X., Drachenberg, J. L., Draper, J. E., Dunkelberger, L. E., Dunlop, J. C., Efimov, L. G., Elsey, N., Engelage, J., Eppley, G., Esha, R., Esumi, S., Evdokimov, O., Ewigleben, J., Eyser, O., Fatemi, R., Fazio, S., Federic, P., Federicova, P., Fedorisin, J., Feng, Z., Filip, P., Finch, E., Fisyak, Y., Flores, C. E., Fujita, J., Fulek, L., Gagliardi, C. A., Garand, D., Geurts, F., Gibson, A., Girard, M., Grosnick, D., Gunarathne, D. S., Guo, Y., Gupta, A., Gupta, S., Guryn, W., Hamad, A. I., Hamed, A., Harlenderova, A., Harris, J. W., He, L., Heppelmann, S., Hirsch, A., Hoffmann, G. W., Horvat, S., Huang, B., Huang, T., Huang, H. Z., Huang, X., Humanic, T. J., Huo, P., Igo, G., Jacobs, W. W., Jentsch, A., Jia, J., Jiang, K., Jowzaee, S., Judd, E. G., Kabana, S., Kalinkin, D., Kang, K., Kauder, K., Ke, H. W., Keane, D., Kechechyan, A., Khan, Z., Kikoła, D. P., Kisel, I., Kisiel, A., Klein, S. R., Kochenda, L., Kocmanek, M., Kollegger, T., Kosarzewski, L. K., Kraishan, A. F., Kravtsov, P., Krueger, K., Kulathunga, N., Kumar, L., Kvapil, J., Kwasizur, J. H., Lacey, R., Landgraf, J. M., Landry, K. D., Lauret, J., Lebedev, A., Lednicky, R., Lee, J. H., Li, W., Li, X., Li, C., Li, Y., Lidrych, J., Lin, T., Lisa, M. A., Liu, Y., Liu, F., Liu, H., Liu, P., Ljubicic, T., Llope, W. J., Lomnitz, M., Longacre, R. S., Luo, S., Luo, X., Ma, G. L., Ma, Y. G., Ma, L., Ma, R., Magdy, N., Majka, R., Mallick, D., Margetis, S., Markert, C., Matis, H. S., Meehan, K., Mei, J. C., Miller, Z. W., Minaev, N. G., Mioduszewski, S., Mishra, D., Mizuno, S., Mohanty, B., Mondal, M. M., Morozov, D. A., Mustafa, M. K., Nasim, Md., Nayak, T. K., Nelson, J. M., Nie, M., Nigmatkulov, G., Niida, T., Nogach, L. V., Nonaka, T., Nurushev, S. B., Odyniec, G., Ogawa, A., Oh, K., Okorokov, V. A., Olvitt Jr., D., Page, B. S., Pak, R., Pandit, Y., Panebratsev, Y., Pawlik, B., Pei, H., Perkins, C., Pile, P., Pluta, J., Poniatowska, K., Porter, J., Posik, M., Poskanzer, A. M., Pruthi, N. K., Przybycien, M., Putschke, J., Qiu, H., Quintero, A., Ramachandran, S., Ray, R. L., Reed, R., Rehbein, M. J., Ritter, H. G., Roberts, J. B., Rogachevskiy, O. V., Romero, J. L., Roth, J. D., Ruan, L., Rusnak, J., Rusnakova, O., Sahoo, N. R., Sahu, P. K., Salur, S., Sandweiss, J., Saur, M., Schambach, J., Schmah, A. M., Schmidke, W. B., Schmitz, N., Schweid, B. R., Seger, J., Sergeeva, M., Seyboth, P., Shah, N., Shahaliev, E., Shanmuganathan, P. V., Shao, M., Sharma, A., Sharma, M. K., Shen, W. Q., Shi, Z., Shi, S. S., Shou, Q. Y., Sichtermann, E. P., Sikora, R., Simko, M., Singha, S., Skoby, M. J., Smirnov, N., Smirnov, D., Solyst, W., Song, L., Sorensen, P., Spinka, H. M., Srivastava, B., Stanislaus, T. D. S., Strikhanov, M., Stringfellow, B., Sugiura, T., Sumbera, M., Summa, B., Sun, Y., Sun, X. M., Sun, X., Surrow, B., Svirida, D. N., Tang, A. H., Tang, Z., Taranenko, A., Tarnowsky, T., Tawfik, A., Thäder, J., Thomas, J. H., Timmins, A. R., Tlusty, D., Todoroki, T., Tokarev, M., Trentalange, S., Tribble, R. E., Tribedy, P., Tripathy, S. K., Trzeciak, B. A., Tsai, O. D., Ullrich, T., Underwood, D. G., Upsal, I., Van Buren, G., van Nieuwenhuizen, G., Vasiliev, A. N., Videbæk, F., Vokal, S., Voloshin, S. A., Vossen, A., Wang, G., Wang, Y., Wang, F., Webb, J. C., Webb, G., Wen, L., Westfall, G. D., Wieman, H., Wissink, S. W., Witt, R., Wu, Y., Xiao, Z. G., Xie, W., Xie, G., Xu, J., Xu, N., Xu, Q. H., Xu, Y. F., Xu, Z., Yang, Y., Yang, Q., Yang, C., Yang, S., Ye, Z., Yi, L., Yip, K., Yoo, I. -K., Yu, N., Zbroszczyk, H., Zha, W., Zhang, Z., Zhang, X. P., Zhang, J. B., Zhang, S., Zhang, J., Zhang, Y., Zhao, J., Zhong, C., Zhou, L., Zhou, C., Zhu, X., Zhu, Z., Zyzak, M.
The STAR Collaboration reports on the photoproduction of $\pi^+\pi^-$ pairs in gold-gold collisions at a center-of-mass energy of 200 GeV/nucleon-pair. These pion pairs are produced when a nearly-real photon emitted by one ion scatters from the other
Externí odkaz:
http://arxiv.org/abs/1702.07705