Results 101 to 110 of about 910,791 (369)
Properties of the Binary Neutron Star Merger GW170817 [PDF]
, 2018 On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic ...The Ligo Scientific Collaboration, The Virgo Collaboration, B. Abbott, R. Abbott, T. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. Adhikari, V. Adya, C. Affeldt, B. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. Aguiar, L. Aiello, A. Ain, P. Ajith, B. Allen, G. Allen, A. Allocca, M. Aloy, P. Altin, A. Amato, A. Ananyeva, S. Anderson, W. Anderson, S. Angelova, S. Antier, S. Appert, K. Arai, M. Araya, J. Areeda, M. Arène, N. Arnaud, K. Arun, S. Ascenzi, G. Ashton, M. Ast, S. Aston, P. Astone, D. V. Atallah, F. Aubin, P. Aufmuth, C. Aulbert, K. AultONeal, C. Austin, A. Ávila-Álvarez, S. Babak, P. Bacon, F. Badaracco, M. Bader, S. Bae, P. Baker, F. Baldaccini, G. Ballardin, S. Ballmer, S. Banagiri, J. Barayoga, S. Barclay, B. Barish, D. Barker, K. Barkett, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, I. Bartos, R. Bassiri, A. Basti, J. Batch, M. Bawaj, J. Bayley, M. Bazzan, B. B'ecsy, C. Beer, M. Bejger, I. Belahcene, A. Bell, D. Beniwal, M. Bensch, B. Berger, G. Bergmann, S. Bernuzzi, J. Bero, C. Berry, D. Bersanetti, A. Bertolini, J. Betzwieser, R. Bhandare, I. Bilenko, S. Bilgili, G. Billingsley, C. Billman, J. Birch, R. Birney, O. Birnholtz, S. Biscans, S. Biscoveanu, A. Bisht, M. Bitossi, M. Bizouard, J. Blackburn, J. Blackman, C. Blair, D. Blair, R. Blair, S. Bloemen, O. Bock, N. Bode, M. Boer, Y. Boetzel, G. Bogaert, A. Bohé, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, C. Booth, R. Bork, V. Boschi, S. Bose, K. Bossie, V. Bossilkov, J. Bosveld, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. Brady, A. Bramley, M. Branchesi, J. Brau, T. Briant, F. Brighenti, A. Brillet, M. Brinkmann, V. Brisson, P. Brockill, A. Brooks, D. Brown, S. Brunett, C. Buchanan, A. Buikema, T. Bulik, H. Bulten, A. Buonanno, D. Buskulic, C. Buy, R. Byer, M. Cabero, L. Cadonati, G. Cagnoli, C. Cahillane, J. C. Bustillo, T. Callister, E. Calloni, J. Camp, M. Canepa, P. Canizares, K. Cannon, H. Cao, J. Cao, C. Capano, E. Capocasa, F. Carbognani, S. Caride, M. Carney, Gregorio Carullo, J. C. Diaz, C. Casentini, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, C. Cepeda, P. Cerd'a-Dur'an, G. Cerretani, E. Cesarini, O. Chaibi, S. Chamberlin, M. Chan, S. Chao, P. Charlton, E. Chase, É. Chassande-Mottin, D. Chatterjee, K. Chatziioannou, B. Cheeseboro, H. Chen, X. Chen, Y. Chen, H.-P. Cheng, H. Chia, A. Chincarini, A. Chiummo, T. Chmiel, H. Cho, M. Cho, J. Chow, N. Christensen, Q. Chu, A. J. Chua, S. Chua, K. Chung, S. Chung, G. Ciani, A. Ciobanu, R. Ciolfi, F. Cipriano, C. Cirelli, A. Cirone, F. Clara, J. Clark, P. Clearwater, F. Cleva, C. Cocchieri, E. Coccia, P. Cohadon, D. Cohen, A. Colla, C. Collette, C. Collins, L. Cominsky, M. Constancio, L. Conti, S. Cooper, P. Corban, T. Corbitt, I. Cordero-Carri'on, K. Corley, N. Cornish, A. Corsi, S. Cortese, C. Costa, R. Cotesta, M. Coughlin, S. Coughlin, J. Coulon, S. Countryman, P. Couvares, P. Covas, E. Cowan, D. Coward, M. Cowart, D. Coyne, R. Coyne, J. Creighton, T. Creighton, J. Cripe, S. Crowder, T. Cullen, A. Cumming, L. Cunningham, E. Cuoco, T. D. Canton, G. D'alya, Beatrice D'Angelo, S. Danilishin, S. D’Antonio, K. Danzmann, A. Dasgupta, C. F. S. Costa, V. Dattilo, I. Dave, M. Davier, D. Davis, E. Daw, B. Day, D. DeBra, M. Deenadayalan, J. Degallaix, M. D. Laurentis, S. Del'eglise, W. D. Pozzo, N. Demos, T. Denker, T. Dent, R. Pietri, J. Derby, V. Dergachev, R. Rosa, C. Rossi, R. DeSalvo, O. D. Varona, S. Dhurandhar, M. D'iaz, T. Dietrich, L. Fiore, M. Giovanni, T. D. Girolamo, A. Lieto, B. Ding, S. D. Pace, I. Palma, F. Renzo, A. Dmitriev, Zoheyr Doctor, V. Dolique, F. Donovan, K. Dooley, S. Doravari, I. Dorrington, M. D. Álvarez, T. Downes, M. Drago, C. Dreissigacker, J. Driggers, Z. Du, R. Dudi, P. Dupej, S. Dwyer, P. Easter, T. Edo, M. Edwards, A. Effler, H. Eggenstein, P. Ehrens, J. Eichholz, S. Eikenberry, M. Eisenmann, R. Eisenstein, R. Essick, H. Estellés, D. Estevez, Z. Etienne, T. Etzel, M. Evans, T. Evans, V. Fafone, H. Fair, S. Fairhurst, X. Fan, S. Farinon, B. Farr, W. Farr, E. Fauchon-Jones, Marc Favata, M. Fays, C. Fee, H. Fehrmann, J. Feicht, M. Fejer, F. Feng, Á. Fernández-Galiana, I. Ferrante, E. Ferreira, F. Ferrini, F. Fidecaro, I. Fiori, D. Fiorucci, M. Fishbach, R. Fisher, J. Fishner, M. Fitz-Axen, R. Flaminio, M. Fletcher, H. Fong, J. Font, P. Forsyth, S. Forsyth, J. Fournier, S. Frasca, F. Frasconi, Z. Frei, A. Freise, R. Frey, V. Frey, P. Fritschel, V. Frolov, P. Fulda, M. Fyffe, H. Gabbard, B. Gadre, S. Gaebel, J. Gair, L. Gammaitoni, M. Ganija, S. Gaonkar, A. García, C. Garc'ia-Quir'os, F. Garufi, B. Gateley, S. Gaudio, G. Gaur, V. Gayathri, G. Gemme, E. Génin, A. Gennai, D. George, J. George, L. Gergely, V. Germain, S. Ghonge, A. Ghosh, A. Ghosh, S. Ghosh, B. Giacomazzo, J. Giaime, K. Giardina, A. Giazotto, K. Gill, G. Giordano, L. Glover, E. Goetz, R. Goetz, B. Goncharov, G. Gonz'alez, J. M. Castro, A. Gopakumar, M. Gorodetsky, S. Gossan, M. Gosselin, R. Gouaty, A. Grado, C. Graef, M. Granata, A. Grant, S. Gras, C. Gray, G. Greco, A. Green, R. Green, E. Gretarsson, P. Groot, H. Grote, S. Grunewald, P. Gruning, G. Guidi, H. Gulati, X. Guo, A. Gupta, M. Gupta, K. Gushwa, E. Gustafson, R. Gustafson, O. Halim, B. Hall, E. Hall, E. Hamilton, H. Hamilton, G. Hammond, M. Haney, M. Hanke, J. Hanks, C. Hanna, M. Hannam, O. Hannuksela, J. Hanson, T. Hardwick, J. Harms, G. Harry, I. Harry, M. Hart, C. Haster, K. Haughian, J. Healy, A. Heidmann, M. Heintze, H. Heitmann, P. Hello, G. Hemming, M. Hendry, I. Heng, J. Hennig, A. Heptonstall, F. Hernandez, M. Heurs, S. Hild, T. Hinderer, D. Hoak, S. Hochheim, D. Hofman, N. Holland, K. Holt, D. Holz, P. Hopkins, C. Horst, J. Hough, E. Houston, E. Howell, A. Hreibi, E. Huerta, D. Huet, B. Hughey, M. Hulko, S. Husa, S. Huttner, T. Huynh--Dinh, A. Iess, N. Indik, C. Ingram, R. Inta +499 moresemanticscholar +1 more sourcePROPERTIES OF NEUTRON STARS [PDF]
Compact Stars, 2004 I review attempts made to determine the properties of neutron stars. I focus on constraints on the maximum mass that a neutron star can have, and on attempts to measure neutron-star radii. So far, there appears to be only one neutron star for which there is strong evidence that its mass is above the canonical 1.4 Msun, viz., Vela X-1, for which a mass ...openaire +2 more sources3D Printed Ultra‐Fast Plastic Scintillators Based on Perovskite‐Photocurable Polymer Composite
Advanced Functional Materials, Volume 35, Issue 12, March 18, 2025.The demand for radiation detection is increasing in a number of fields, including high‐energy physics, medical imaging, and homeland security. This study serves to demonstrate the potential for the fabrication of fast perovskite‐based scintillators with complex shapes via stereolithographic additive manufacturing, representing a new path toward the ...Antonella Giuri, Amal C Chekkallur, Mario Calora, Rosanna Mastria, Loris Martinazzoli, Etiennette Auffray, Sanosh Kunjalukkal Padmanabhan, Sara Carturan, Sandra Moretto, Gianluca Quarta, Lucio Calcagnile, Matteo Polo, Alberto Quaranta, Alfonso Maffezzoli, Anna Paola Caricato, Aurora Rizzo, Carola Esposito Corcione +16 morewiley +1 more sourceElectromagnetic extraction of energy from black hole-neutron star
binaries
, 2011 The coalescence of black hole-neutron star binaries is expected to be a
principal source of gravitational waves for the next generation of detectors,
Advanced LIGO and Advanced Virgo.Basko, Blandford, Cline, Damour, Fermi GLAST Burst Monitor (GBM), Janna Levin, McGill SGR/AXP Online Catalog, McWilliams, Misner, Rosswog, Sean T. McWilliams, Swift's Burst Alert Telescope (BAT), Thorne, Özel +13 morecore +1 more sourceControl of Ferromagnetism of Vanadium Oxide Thin Films by Oxidation States
Advanced Functional Materials, EarlyView.The nonstoichiometric VOx exhibits a distinct ferromagnetic hysteresis loop and demonstrates a high magnetic susceptibility (χ=dMdH$ = \frac{{dM}}{{dH}}\;$∼10). Micromagnetic simulations show the results of the “partial volume fraction ferromagnetic phase model” for VOx/Co/Pt structure.Kwonjin Park, Jaeyong Cho, Soobeom Lee, Jaehun Cho, Jae‐Hyun Ha, Jinyong Jung, Dongryul Kim, Won‐Chang Choi, Jung‐Il Hong, Chun‐Yeol You +9 morewiley +1 more sourceBound Debris Expulsion from Neutron Star Merger Remnants
The Astrophysical Journal, 2023 Many studies have found that neutron star mergers leave a fraction of the stars’ mass in bound orbits surrounding the resulting massive neutron star or black hole. This mass is a site of r -process nucleosynthesis and can generate a wind that contributes Yossef Zenati, Julian H. Krolik, Leonardo R. Werneck, Ariadna Murguia-Berthier, Zachariah B. Etienne, Scott C. Noble, Tsvi Piran +6 moredoaj +1 more sourceObservational constraints on the neutron star mass distribution [PDF]
, 1994 Radio observations of neutron star binary pulsar systems have constrained
strongly the masses of eight neutron stars. Assuming neutron star masses are
uniformly distributed between lower and upper bounds $m_l$ and $m_u$, the
observations determine with ...A. Abramovici, A. Wolszczan, C. Cutler, C.E. Rhoades, F. Verbunt, J.B. Hartle, J.H. Taylor, L.S. Finn, Lee Samuel Finn, M.F. Ryba, P.C. Joss, R. Narayan, S.E. Thorsett, S.E. Woosley, S.L. Shapiro, T.A. Prince +15 morecore +2 more sources
