Stuart Shapiro

University of Illinois at Urbana-Champaign

Stellar Astronomy and Astrophysics

2017

Lunan Sun, Vasileios Paschalidis, Milton Ruiz, and Stuart L. Shapiro (2017): Magnetorotational Collapse of Supermassive Stars: Black Hole Formation, Gravitational Waves, and Jets, Physical Review D, American Physical Society (APS), Vol 96, Num 4, pp043006
Stuart L. Shapiro (2017): Black Holes, Disks, and Jets Following Binary Mergers and Stellar Collapse: The Narrow Range of Electromagnetic Luminosities and Accretion Rates, Physical Review D, American Physical Society (APS), Vol 95, Num 10, pp101303
Antonios Tsokaros, Milton Ruiz, Vasileios Paschalidis, Stuart L. Shapiro, Luca Baiotti, and Koji Uryu (2017): Gravitational Wave Content and Stability of Uniformly, Rotating, Triaxial Neutron Stars in General Relativity, Physical Review D, American Physical Society (APS), Vol 95, Num 12, pp124057

2016

Milton Ruiz, Ryan N. Lang, Vasileios Paschalidis, and Stuart L. Shapiro (2016): Binary Neutron Star Mergers: A Jet Engine for Short Gamma-Ray Burst, ApJ, American Astronomical Society, Vol 824, Num 1, ppL6

2015

Vasileios Paschalidis, Milton Ruiz, and Stuart L. Shapiro (2015): Relativistic Simulations of Black Hole-Neutron Star Coalescence: The Jet Emerges, The Astrophysical Journal Letters, The American Astronomical Society, Vol 806, Num 1, ppL14

2014

J Aasi and B P Abbott and R Abbott and T Abbott and M R Abernathy and T Accadia and F Acernese and K Ackley and C Adams and T Adams and PAddesso and R X Adhikari and C Affeldt and M Agathos and N Aggarwal and O D Aguiar and A Ain and P Ajith and A Alemic and B Allen and AAllocca and D Amariutei and M Andersen and R Anderson and S B Anderson and W G Anderson and K Arai and M C Araya and C Arceneaux and JAreeda and S M Aston and P Astone and P Aufmuth and C Aulbert and L Austin and B E Aylott and S Babak and P T Baker and G Ballardin and S WBallmer and J C Barayoga and M Barbet and B C Barish and D Barker and F Barone and B Barr and L Barsotti and M Barsuglia and M ABarton and I Bartos and R Bassiri and A Basti and J C Batch and J Bauchrowitz and Th S Bauer and B Behnke and M Bejger and M G Beker and CBelczynski and A S Bell and C Bell and G Bergmann and D Bersanetti and A Bertolini and J Betzwieser and P T Beyersdorf and I ABilenko and G Billingsley and J Birch and S Biscans and M Bitossi and M A Bizouard and E Black and J K Blackburn and L Blackburn and DBlair and S Bloemen and M Blom and O Bock and T P Bodiya and M Boer and G Bogaert and C Bogan and C Bond and F Bondu and L Bonelli and RBonnand and R Bork and M Born and V Boschi and Sukanta Bose and L Bosi and C Bradaschia and P R Brady and V B Braginsky and MBranchesi and J E Brau and T Briant and D O Bridges and A Brillet and M Brinkmann and V Brisson and A F Brooks and D A Brown and D DBrown and F Brückner and S Buchman and T Bulik and H J Bulten and A Buonanno and R Burman and D Buskulic and C Buy and L Cadonati and GCagnoli and J Calderón Bustillo and E Calloni and J B Camp and P Campsie and K C Cannon and B Canuel and J Cao and C D Capano and FCarbognani and L Carbone and S Caride and A Castiglia and S Caudill and M Cavaglià and F Cavalier and R Cavalieri and C Celerier and GCella and C Cepeda and E Cesarini and R Chakraborty and T Chalermsongsak and S J Chamberlin and S Chao and P Charlton and EChassande-Mottin and X Chen and Y Chen and A Chincarini and A Chiummo and H S Cho and J Chow and N Christensen and Q Chu and S S YChua and S Chung and G Ciani and F Clara and J A Clark and F Cleva and E Coccia and P-F Cohadon and A Colla and C Collette and M Colombini and LCominsky and M Constancio Jr and A Conte and D Cook and T R Corbitt and M Cordier and N Cornish and A Corpuz and A Corsi and C A Costa and MW Coughlin and S Coughlin and J-P Coulon and S Countryman and P Couvares and D M Coward and M Cowart and D C Coyne and R Coyne and KCraig and J D E Creighton and S G Crowder and A Cumming and L Cunningham and E Cuoco and K Dahl and T Dal Canton and M Damjanic and S LDanilishin and S D’Antonio and K Danzmann and V Dattilo and H Daveloza and M Davier and G S Davies and E J Daw and R Day and T Dayanga and GDebreczeni and J Degallaix and S Deléglise and W Del Pozzo and T Denker and T Dent and H Dereli and V Dergachev and R De Rosa and R TDeRosa and R DeSalvo and S Dhurandhar and M Díaz and L Di Fiore and A Di Lieto and I Di Palma and A Di Virgilio and A Donath and FDonovan and K L Dooley and S Doravari and S Dossa and R Douglas and T P Downes and M Drago and R W P Drever and J C Driggers and Z Du and SDwyer and T Eberle and T Edo and M Edwards and A Effler and H Eggenstein and P Ehrens and J Eichholz and S S Eikenberry and G Endrőczi and REssick and T Etzel and M Evans and T Evans and M Factourovich and V Fafone and S Fairhurst and Q Fang and S Farinon and B Farr and W MFarr and M Favata and H Fehrmann and M M Fejer and D Feldbaum and F Feroz and I Ferrante and F Ferrini and F Fidecaro and L S Finn and IFiori and R P Fisher and R Flaminio and J-D Fournier and S Franco and S Frasca and F Frasconi and M Frede and Z Frei and A Freise and RFrey and T T Fricke and P Fritschel and V V Frolov and P Fulda and M Fyffe and J Gair and L Gammaitoni and S Gaonkar and F Garufi and NGehrels and G Gemme and E Genin and A Gennai and S Ghosh and J A Giaime and K D Giardina and A Giazotto and C Gill and J Gleason and EGoetz and R Goetz and L Gondan and G González and N Gordon and M L Gorodetsky and S Gossan and S Goßler and R Gouaty and C Gräf and P BGraff and M Granata and A Grant and S Gras and C Gray and R J S Greenhalgh and A M Gretarsson and P Groot and H Grote and K Grover and SGrunewald and G M Guidi and C Guido and K Gushwa and E K Gustafson and R Gustafson and D Hammer and G Hammond and M Hanke and J Hanks and CHanna and J Hanson and J Harms and G M Harry and I W Harry and E D Harstad and M Hart and M T Hartman and C-J Haster and K Haughian and AHeidmann and M Heintze and H Heitmann and P Hello and G Hemming and M Hendry and I S Heng and A W Heptonstall and M Heurs and MHewitson and S Hild and D Hoak and K A Hodge and K Holt and S Hooper and P Hopkins and D J Hosken and J Hough and E J Howell and Y Hu and BHughey and S Husa and S H Huttner and M Huynh and T Huynh-Dinh and D R Ingram and R Inta and T Isogai and A Ivanov and B R Iyer and KIzumi and M Jacobson and E James and H Jang and P Jaranowski and Y Ji and F Jiménez-Forteza and W W Johnson and D I Jones and R Jones and RJ G Jonker and L Ju and Haris K and P Kalmus and V Kalogera and S Kandhasamy and G Kang and J B Kanner and J Karlen and M Kasprzack and EKatsavounidis and W Katzman and H Kaufer and K Kawabe and F Kawazoe and F Kéfélian and G M Keiser and D Keitel and D B Kelley and WKells and A Khalaidovski and F Y Khalili and E A Khazanov and C Kim and K Kim and N Kim and N G Kim and Y-M Kim and E J King and P J King and DL Kinzel and J S Kissel and S Klimenko and J Kline and S Koehlenbeck and K Kokeyama and V Kondrashov and S Koranda and W Z Korth and IKowalska and D B Kozak and A Kremin and V Kringel and B Krishnan and A Królak and G Kuehn and A Kumar and P Kumar and R Kumar and L Kuo and AKutynia and P Kwee and M Landry and B Lantz and S Larson and P D Lasky and C Lawrie and A Lazzarini and C Lazzaro and P Leaci and S Leavey and EO Lebigot and C-H Lee and H K Lee and H M Lee and J Lee and M Leonardi and J R Leong and A Le Roux and N Leroy and N Letendre and Y Levin and BLevine and J Lewis and T G F Li and K Libbrecht and A Libson and A C Lin and T B Littenberg and V Litvine and N A Lockerbie and VLockett and D Lodhia and K Loew and J Logue and A L Lombardi and M Lorenzini and V Loriette and M Lormand and G Losurdo and J Lough and M JLubinski and H Lück and E Luijten and A P Lundgren and R Lynch and Y Ma and J Macarthur and E P Macdonald and T MacDonald and BMachenschalk and M MacInnis and D M Macleod and F Magana-Sandoval and M Mageswaran and C Maglione and K Mailand and E Majorana and IMaksimovic and V Malvezzi and N Man and G M Manca and I Mandel and V Mandic and V Mangano and N Mangini and M Mantovani and FMarchesoni and F Marion and S Márka and Z Márka and A Markosyan and E Maros and J Marque and F Martelli and I W Martin and R M Martin and LMartinelli and D Martynov and J N Marx and K Mason and A Masserot and T J Massinger and F Matichard and L Matone and R A Matzner and NMavalvala and N Mazumder and G Mazzolo and R McCarthy and D E McClelland and S C McGuire and G McIntyre and J McIver and K McLin and DMeacher and G D Meadors and M Mehmet and J Meidam and M Meinders and A Melatos and G Mendell and R A Mercer and S Meshkov and CMessenger and P Meyers and H Miao and C Michel and E E Mikhailov and L Milano and S Milde and J Miller and Y Minenkov and C M FMingarelli and C Mishra and S Mitra and V P Mitrofanov and G Mitselmakher and R Mittleman and B Moe and P Moesta and M Mohan and S R PMohapatra and D Moraru and G Moreno and N Morgado and S R Morriss and K Mossavi and B Mours and C M Mow-Lowry and C L Mueller and GMueller and S Mukherjee and A Mullavey and J Munch and D Murphy and P G Murray and A Mytidis and M F Nagy and D Nanda Kumar and INardecchia and L Naticchioni and R K Nayak and V Necula and G Nelemans and I Neri and M Neri and G Newton and T Nguyen and A Nitz and FNocera and D Nolting and M E N Normandin and L K Nuttall and E Ochsner and J O’Dell and E Oelker and J J Oh and S H Oh and F Ohme and POppermann and B O’Reilly and R O’Shaughnessy and C Osthelder and D J Ottaway and R S Ottens and H Overmier and B J Owen and CPadilla and A Pai and O Palashov and C Palomba and H Pan and Y Pan and C Pankow and F Paoletti and R Paoletti and M A Papa and H Paris and APasqualetti and R Passaquieti and D Passuello and M Pedraza and S Penn and A Perreca and M Phelps and M Pichot and M Pickenpack and FPiergiovanni and V Pierro and L Pinard and I M Pinto and M Pitkin and J Poeld and R Poggiani and A Poteomkin and J Powell and J Prasad and SPremachandra and T Prestegard and L R Price and M Prijatelj and S Privitera and G A Prodi and L Prokhorov and O Puncken and MPunturo and P Puppo and J Qin and V Quetschke and E Quintero and G Quiroga and R Quitzow-James and F J Raab and D S Rabeling and IRácz and H Radkins and P Raffai and S Raja and G Rajalakshmi and M Rakhmanov and C Ramet and K Ramirez and P Rapagnani and V Raymond and VRe and J Read and C M Reed and T Regimbau and S Reid and D H Reitze and E Rhoades and F Ricci and K Riles and N A Robertson and F Robinet and ARocchi and M Rodruck and L Rolland and J G Rollins and R Romano and G Romanov and J H Romie and D Rosińska and S Rowan and A Rüdiger and PRuggi and K Ryan and F Salemi and L Sammut and V Sandberg and J R Sanders and V Sannibale and I Santiago-Prieto and E Saracco and BSassolas and B S Sathyaprakash and P R Saulson and R Savage and J Scheuer and R Schilling and R Schnabel and R M S Schofield and ESchreiber and D Schuette and B F Schutz and J Scott and S M Scott and D Sellers and A S Sengupta and D Sentenac and V Sequino and ASergeev and D Shaddock and S Shah and M S Shahriar and M Shaltev and B Shapiro and P Shawhan and D H Shoemaker and T L Sidery and KSiellez and X Siemens and D Sigg and D Simakov and A Singer and L Singer and R Singh and A M Sintes and B J J Slagmolen and J Slutsky and JR Smith and M Smith and R J E Smith and N D Smith-Lefebvre and E J Son and B Sorazu and T Souradeep and L Sperandio and A Staley and JStebbins and J Steinlechner and S Steinlechner and B C Stephens and S Steplewski and S Stevenson and R Stone and D Stops and K AStrain and N Straniero and S Strigin and R Sturani and A L Stuver and T Z Summerscales and S Susmithan and P J Sutton and BSwinkels and M Tacca and D Talukder and D B Tanner and S P Tarabrin and R Taylor and A P M ter Braack and M PThirugnanasambandam and M Thomas and P Thomas and K A Thorne and K S Thorne and E Thrane and V Tiwari and K V Tokmakov and CTomlinson and A Toncelli and M Tonelli and O Torre and C V Torres and C I Torrie and F Travasso and G Traylor and M Tse and D Ugolini and CS Unnikrishnan and A L Urban and K Urbanek and H Vahlbruch and G Vajente and G Valdes and M Vallisneri and J F J van den Brand and CVan Den Broeck and S van der Putten and M V van der Sluys and J van Heijningen and A A van Veggel and S Vass and M Vasúth and RVaulin and A Vecchio and G Vedovato and J Veitch and P J Veitch and K Venkateswara and D Verkindt and S S Verma and F Vetrano and AViceré and R Vincent-Finley and J-Y Vinet and S Vitale and T Vo and H Vocca and C Vorvick and W D Vousden and S P Vyachanin and A Wade and LWade and M Wade and M Walker and L Wallace and M Wang and X Wang and R L Ward and M Was and B Weaver and L-W Wei and M Weinert and A JWeinstein and R Weiss and T Welborn and L Wen and P Wessels and M West and T Westphal and K Wette and J T Whelan and S E Whitcomb and D JWhite and B F Whiting and K Wiesner and C Wilkinson and K Williams and L Williams and R Williams and T Williams and A R Williamson and JL Willis and B Willke and M Wimmer and W Winkler and C C Wipf and A G Wiseman and H Wittel and G Woan and J Worden and J Yablon and IYakushin and H Yamamoto and C C Yancey and H Yang and Z Yang and S Yoshida and M Yvert and A Zadrożny and M Zanolin and J-P Zendri and FanZhang and L Zhang and C Zhao and X J Zhu and M E Zucker and S Zuraw and J Zweizig and M Boyle and B Brügmann and L T Buchman and MCampanelli and T Chu and Z B Etienne and M Hannam and J Healy and I Hinder and L E Kidder and P Laguna and Y T Liu and L London and C OLousto and G Lovelace and I MacDonald and P Marronetti and P Mösta and D Müller and B C Mundim and H Nakano and V Paschalidis and LPekowsky and D Pollney and H P Pfeiffer and M Ponce and M Pürrer and G Reifenberger and C Reisswig and L Santamaría and M A Scheel and SL Shapiro and D Shoemaker and C F Sopuerta and U Sperhake and B Szilágyi and N W Taylor and W Tichy and P Tsatsin and Y Zlochower (2014): The NINJA-2 Project: Detecting and Characterizing Gravitational Waveforms Modelled Using Numerical Binary Black Hole Simulations, Class. Quantum Grav., IOP Publishing, Vol 31, Num 11, pp115004
Milton Ruiz, Vasileios Paschalidis, and Stuart L. Shapiro (2014): Pulsar Spin-Down Luminosity: Simulations in General Relativity, Physical Review D, American Physical Society (APS), Vol 89, Num 8, pp084045
Roman Gold, Vasileios Paschalidis, Milton Ruiz, Stuart L. Shapiro, Zachariah B. Etienne, and Harald P. Pfeiffer (2014): Accretion Disks Around Binary Black Holes of Unequal Mass: General Relativistic MHD Simulations of Postdecoupling and Merger, Physical Review D, American Physical Society (APS), Vol 90, Num 10, pp104030
Roman Gold, Vasileios Paschalidis, Zachariah B. Etienne, Stuart L. Shapiro, and Harald P. Pfeiffer (2014): Accretion Disks Around Binary Black Holes of Unequal Mass: General Relativistic Magnetohydrodynamic Simulations Near Decoupling, Physical Review D, American Physical Society (APS), Vol 89, Num 6, pp064060
Zachariah B. Etienne, John G. Baker, Vasileios Paschalidis, Bernard J. Kelly, and Stuart L. Shapiro (2014): Improved Moving Puncture Gauge Conditions for Compact Binary Evolutions, Physical Review D, American Physical Society (APS), Vol 90, Num 6, pp064032

2013

Ian Hinder and Alessandra Buonanno and Michael Boyle and Zachariah B Etienne and James Healy and Nathan KJohnson-McDaniel and Alessandro Nagar and Hiroyuki Nakano and Yi Pan and Harald P Pfeiffer and Michael Pürrer and ChristianReisswig and Mark A Scheel and Erik Schnetter and Ulrich Sperhake and Bela Szilágyi and Wolfgang Tichy and BarryWardell and Anıl Zenginoğlu and Daniela Alic and Sebastiano Bernuzzi and Tanja Bode and Bernd Brügmann and Luisa TBuchman and Manuela Campanelli and Tony Chu and Thibault Damour and Jason D Grigsby and Mark Hannam and Roland Haas and Daniel AHemberger and Sascha Husa and Lawrence E Kidder and Pablo Laguna and Lionel London and Geoffrey Lovelace and Carlos OLousto and Pedro Marronetti and Richard A Matzner and Philipp Mösta and Abdul Mroué and Doreen Müller and Bruno CMundim and Andrea Nerozzi and Vasileios Paschalidis and Denis Pollney and George Reifenberger and LucianoRezzolla and Stuart L Shapiro and Deirdre Shoemaker and Andrea Taracchini and Nicholas W Taylor and Saul ATeukolsky and Marcus Thierfelder and Helvi Witek and Yosef Zlochower (2013): Error-Analysis and Comparison to Analytical Models of Numerical Waveforms Produced by the NRAR Collaboration, Classical and Quantum Gravity, IOP Publishing, Vol 31, Num 2, pp025012

2012

P Ajith and Michael Boyle and Duncan A Brown and Bernd Brügmann and Luisa T Buchman and Laura Cadonati and ManuelaCampanelli and Tony Chu and Zachariah B Etienne and Stephen Fairhurst and Mark Hannam and James Healy and Ian Hinder and SaschaHusa and Lawrence E Kidder and Badri Krishnan and Pablo Laguna and Yuk Tung Liu and Lionel London and Carlos OLousto and Geoffrey Lovelace and Ilana MacDonald and Pedro Marronetti and Satya Mohapatra and Philipp Mösta and DoreenMüller and Bruno C Mundim and Hiroyuki Nakano and Frank Ohme and Vasileios Paschalidis and Larne Pekowsky and DenisPollney and Harald P Pfeiffer and Marcelo Ponce and Michael Pürrer and George Reifenberger and Christian Reisswig and LucíaSantamaría and Mark A Scheel and Stuart L Shapiro and Deirdre Shoemaker and Carlos F Sopuerta and Ulrich Sperhake and BélaSzilágyi and Nicholas W Taylor and Wolfgang Tichy and Petr Tsatsin and Yosef Zlochower (2012): The NINJA-2 Catalog of Hybrid Post-Newtonian/numerical-Relativity Waveforms for Non-Precessing Black-Hole Binaries, Class. Quantum Grav., IOP Publishing, Vol 29, Num 12, pp124001

NCSA Grants $2.6M in Blue Waters Awards to Illinois Researchers

The National Center for Supercomputing Applications (NCSA) at the University of Illinois at Urbana-Champaign has awarded 3,697,000 node hours (NH) of time on the Blue Waters supercomputer to Illinois researchers from Spring 2017 proposal submissions.The combined value of these awards is over $2.6 million dollars, and through the life of the Blue Waters program, NCSA has awarded over 43 million node hours to UI researchers—a value of nearly $27 million. Some of the time allocated for Blue Waters will go to projects that focus on HIV research, Laser Interferometer Gravitational-Wave Observatory (LIGO) simulations, genomics and global warming research..

17 campus teams to accelerate their research with Blue Waters

Seventeen U of I research teams from a wide range of disciplines have been awarded computational and data resources on the sustained-petascale Blue Waters supercomputer at NCSA. “These diverse projects highlight the breadth of computational research at the University of Illinois,” said Athol Kemball, associate professor of Astronomy and chair of the Illinois allocation review committee. “Illinois has a tremendous pool of talented researchers in fields from political science to chemistry to engineering who can harness the power of Blue Waters to discover and innovate.”.

22 Illinois projects receive time on Blue Waters

The University of Illinois at Urbana-Champaign has awarded access to the Blue Waters supercomputer—which is capable of performing quadrillions of calculations every second and of working with quadrillions of bytes of data—to 22 campus research teams from a wide range of disciplines.The computing and data capabilities of Blue Waters, which is operated by the National Center for Supercomputing Applications (NCSA), will assist researchers in their work on understanding DNA, developing biofuels, simulating climate, and more..

Discovery confirms Einstein prediction; NCSA played role

A billion light years from Earth, two dense objects known as black holes collide at enormous speed, sending giant ripples through the fabric of space-time.Albert Einstein predicted such an event a century ago as part of his theory of relativity, and scientists have been searching for those ripples, known as gravitational waves, ever since.The announcement of their discovery sent waves of excitement around the globe Thursday, including at the National Center for Supercomputing Applications in Urbana, created 30 years ago to help scientists solve enormous computational puzzles like this one..

Gravitational waves detected 100 years after Einstein’s prediction

For the first time, scientists have observed ripples in the fabric of spacetime called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major prediction of Albert Einstein’s 1915 general theory of relativity and opens an unprecedented new window onto the cosmos. ... The gravitational waves were detected on Sept. 14, 2015, at 5:51 a.m. Eastern Daylight Time (9:51 UTC) by both of the twin Laser Interferometer Gravitational-wave Observatory (LIGO) detectors, located in Livingston, La., and Hanford, Wash. The LIGO Observatories are funded by the National Science Foundation, and were conceived, built, and are operated by Caltech and Massachusetts Institute of Technology. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration (which includes the GEO Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy) and the Virgo Collaboration using data from the two LIGO detectors..

Leggo my LIGO

After LIGO detected gravitational waves a few months ago (detected in September 2015 but announced in February 2016), LIGO and gravitational waves became almost household words. However, did you know that the revolutionary observations couldn’t have been made without the help of the U of I? ... In recognition of his work in getting NSF funding to build these supercomputers and the benefits thereof, Professor Smarr was awarded the Golden Goose award by the Association of American Universities back in February of 2014. The award is presented once a year to honor federally-funded research which has lead to major breakthroughs in science. Any researcher who has produced something within the previous 60 years is eligible. The fact that Professor Smarr received this award is a testament to the importance of the NCSA and its capabilities..