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ATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,UniversityATUL KEDIA
Atul Kedia. PhD Candidate at the University of Notre Dame. Physics Department, University of Notre Dame, Indiana, USA Pronouns: he/him/his akedia@nd.edu . Researcher of computational and theoretical astrophysics and cosmology, teacher of physics, and much more!! RESEARCH BY ATUL KEDIA Binary neutron star mergers. Mergers of a pair of neutron stars for different equations of state (EoS) starting from a single polytropic (first simulation) to Quark-Hadron Crossover EoS from Baym et al. (2019).Simulations performed by forming initial data using LORENE and evolution using Einstein Toolkit. Plot specifications: Timescale is in "Cactus Units", where 1000 CU ≈ 5 milliseconds. ATUL KEDIA'S PUBLICATIONS Get in touch. Please feel free to get in touch with me. akedia@nd.edu; 341 Nieuwland Science Hall Notre Dame, Indiana 46556ATUL KEDIA
Atul Kedia PhysicsPhDCandidate UniversityofNotreDame Website:atulkedia93.github.io GoogleScholarpage Email: akedia@nd.edu Education Present Ph.D. Candidate,University* Curriculum Vitae
ATUL KEDIA
THIRD YEAR GRADUATE STUDENT INTERESTS: COSMOLOGY AND ASTROPHYSICS DEPARTMENT OF PHYSICS UNIVERSITY OF NOTRE DAME, USAakedia@nd.edu
PROJECTS
PRIMORDIAL MAGNETIC FIELDS IN THE BIG BANG NUCLEOSYNTHESIS STAGEOF THE UNIVERSE
January 2017 - present _ Prof. Grant Mathews, University of Notre Dame _ SCALE OF HOMOGENEITY OF THE COSMOS May 2014 - December 2015 _ Prof. Subhabrata Majumdar, Tata Institute of FundamentalResearch _
STABILITY OF NON-RELATIVISTIC MAGNETIZED ASTROPHYSICAL JETS May 2015 - July 2015 _ Prof. Dinshaw Balsara, University of Notre Dame _RESEARCH INTERESTS
* Theoretical and computational cosmology and astrophysicsDetails
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