Results 21 to 30 of about 4,107,153 (300)

Tight multimessenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light-curve synthesis [PDF]

Monthly notices of the Royal Astronomical Society, 2021
We present a rapid analytic framework for predicting kilonova light curves following neutron star (NS) mergers, where the main input parameters are binary-based properties measurable by gravitational wave detectors (chirp mass and mass ratio, orbital ...
M. Nicholl, B. Margalit, P. Schmidt, Graham P. Smith, E. Ridley, J. Nuttall   +5 more
semanticscholar   +1 more source

GW170817: Measurements of Neutron Star Radii and Equation of State. [PDF]

Physical Review Letters, 2018
On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system.
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, 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, 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. Bécsy, 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. 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. Bohe, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, C. D. Booth, R. Bork, V. Boschi, S. Bose, 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, Daniel Brown, S. Brunett, C. Buchanan, A. Buikema, T. Bulik, H. Bulten, A. Buonanno, 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, Junwei Cao, C. Capano, E. Capocasa, F. Carbognani, S. Caride, M. Carney, G. Carullo, J. C. Diaz, C. Casentini, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, C. Cepeda, P. Cerdá-Durán, G. Cerretani, E. Cesarini, O. Chaibi, S. Chamberlin, M. Chan, S. Chao, P. Charlton, E. Chase, E. Chassande-Mottin, D. Chatterjee, K. Chatziioannou, B. Cheeseboro, Hsiao-Wen Chen, Xingang Chen, Yanbei Chen, Hai-Ping 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, 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-Carrión, K. Corley, N. Cornish, A. Corsi, S. Cortese, C. A. Costa, R. Cotesta, M. Coughlin, S. 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. Dalya, 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. Deléglise, W. D. Pozzo, N. Demos, T. Denker, T. Dent, R. Pietri, J. Derby, V. Dergachev, R. D. Rosa, C. Rossi, R. DeSalvo, O. D. Varona, S. Dhurandhar, M. Díaz, T. Dietrich, L. Fiore, M. Giovanni, T. D. Girolamo, A. D. Lieto, B. Ding, S. D. Pace, I. Palma, F. Renzo, A. Dmitriev, Zoheyr Doctor, V. Dolique, F. Donovan, K. Dooley, K. Dooley, S. Doravari, I. Dorrington, M. D. Álvarez, T. Downes, M. Drago, C. Dreissigacker, J. Driggers, Z. Du, 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, Xiaodan 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. García-Quirós, 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, Shaon Ghosh, B. Giacomazzo, J. Giaime, J. Giaime, K. Giardina, A. Giazotto, K. Gill, G. Giordano, L. Glover, E. Goetz, R. Goetz, B. Goncharov, G. González, 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, Arnab Sen 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, W. C. Ho, 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   +499 more
semanticscholar   +1 more source

Microfluidics: A Novel Approach for Dehydration Protein Droplets

Biosensors, 2021
The equation of state of colloids plays an important role in the modelling and comprehension of industrial processes, defining the working conditions of processes such as drying, filtration, and mixing.
Van Nhat Pham, Dimitri Radajewski, Isaac Rodríguez-Ruiz, Sebastien Teychene   +3 more
doaj   +1 more source

Kinetic equation consistent with the equation of state of nuclear matter [PDF]

, 1998
A kinetic equation which combines the quasiparticle drift of Landau's equation with a dissipation governed by a nonlocal and noninstant scattering integral in the spirit of Snider's equation for gases is derived.
Alm, Baerwinkel, Baerwinkel, Bertsch, Bogoliubov, Bornath, Chapman, Danielewicz, Danielewicz, de Haan, de Haan, de Haan, Green, Hirschfelder, Kawasaki, Kortemeyer, Köhler, Malfliet, Morawetz, Nacher, Nacher, Snider, Stöcker, Špička, Špička, Špička, Špička   +26 more
core   +2 more sources

Radial Oscillations in Neutron Stars from Unified Hadronic and Quarkyonic Equation of States

Galaxies, 2023
We study radial oscillations in non-rotating neutron stars by considering the unified equation of states (EoSs), which support the 2 M⊙ star criterion.
Souhardya Sen, Shubham Kumar, Athul Kunjipurayil, Pinku Routaray, Sayantan Ghosh, Probit J. Kalita, Tianqi Zhao, Bharat Kumar   +7 more
doaj   +1 more source

Uncertainty quantification for a multi-phase carbon equation of state model

Journal of Applied Physics, 2022
Many physics models have tunable parameters that are calibrated by matching the model output to experimental or calculated data. However, given that calibration data often contain uncertainty and that different model parameter sets might result in a very
B. A. Lindquist, R. Jadrich
semanticscholar   +1 more source

Equation of state from lattice QCD [PDF]

, 2005
Recent results on the equation of state from lattice QCD are reviewed. The lattice technique and previous results are shortly discussed. New results for physical quark masses and two sets of lattice spacings are presented.
Katz, S. D.
core   +3 more sources

Induced gravitational wave interpretation of PTA data: a complete study for general equation of state [PDF]

Journal of Cosmology and Astroparticle Physics
We thoroughly study the induced gravitational wave interpretation of the possible gravitational wave background reported by PTA collaborations, considering the unknown equation of state w of the early universe.
Guillem Domènech, Shi Pi, Ao Wang, Jianing Wang   +3 more
semanticscholar   +1 more source

Neural simulation-based inference of the neutron star equation of state directly from telescope spectra [PDF]

Journal of Cosmology and Astroparticle Physics
Neutron stars provide a unique opportunity to study strongly interacting matter under extreme density conditions. The intricacies of matter inside neutron stars and their equation of state are not directly visible, but determine bulk properties, such as ...
Len Brandes, Chirag Modi, A. Ghosh, D. Farrell, Lee Lindblom, L. Heinrich, Andrew W. Steiner, Fridolin Weber, D. Whiteson   +8 more
semanticscholar   +1 more source

An inflationary equation-of-state

International Journal of Modern Physics D, 2023
In this paper, we have studied inflationary paradigm through an inflationary equation-of-state. With a single parameter equation-of-state as a function of the scalar field responsible for accelerated expansion, we find an observationally viable model satisfying all the constraints as laid down by the recent observations.
openaire   +2 more sources