Tousif Islam (তৌসিফ ইসলাম)
Talks
Summary : 23 Seminars, 17 Conference Talks, 8 Conference Posters
Seminars & Colloquia
- ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
LISA Consortium Talks
[Dec 2022] - ‘One model to rule all regimes : surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
Strong Gravity Seminar, Perimeter Institute for Theoretical Physics
[Dec 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
Black Hole Initiative, Harvard University
[November 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
GW Group Meeting, John Hopkins Universty
[October 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
GW Group Meeting, Penn State
[October 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
LIGO Seminar, MIT
[Sep 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
GW Group Meeting, Center for Computational Astrophysics, Flatiron Institue
[Aug 2022] - ‘High-accuracy inference of binary black hole source properties using numerical relativity surrogate models’,
Tata Institute for Fundametal Research (TIFR) Astrophysics Seminar
[July 2022] - ‘High-accuracy inference of binary black hole source properties using numerical relativity surrogate models’,
Indian Institute of Technology (IIT) Bombay Physics Seminar
[July 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
International Centre for Theoretical Sciences - TIFR Institute Astrophysical Relativity Seminar
[June 2022] - ‘High-accuracy inference of binary black hole source properties using numerical relativity surrogate models’,
Raman Research Institute Theoretical Physics Seminar
[June 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
University of Mississippi Gravity Seminar
[June 2022] - ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
University of California Santa Barbara Gravitation Wave Seminar
[May 2022] - ‘Tuning perturbation theory waveforms to Numerical Relativity Data : Lessons from EMRISurrogate projects’,
Numerical Relativity Monthly Community Call
[February 2022] - ‘Eccentric binary black hole surrogate models for the gravitational waveform’,
Institute for Pure and Applied Mathematics, University of California Los Angeles
[November 2021] - ‘Testing the no-hair theorem of binary black holes using gravitational waves’,
Kavli Institute of Theoretical Physics, University of California Santa Barbara
[October 2021] - ‘Questioning Einstein : Only to believe him more’,
Indian Institute of Science Education and Research (IISER) Kolkata, Physics Journal Club Talks
[October 2021] - ‘Gravitational multipolar radiation from binary black hole coalsences: waveform modelling and applicability’,
Proposal Talk, UMass Dartmouth
[May 2021] - ‘Eccentric binary black hole surrogate models for the gravitational waveform: comparable to intermediate mass ratio binaires’,
Monash University
[Apr 2021] - ‘Testing the “no-hair” nature of binary black holes using the consistency of multipolar gravitational radiation’,
Center for Computational Astrophysics, Flatiron Institute, Simons Foundation
[Apr 2021] - ‘Intermediate mass ratio inspirals (IMRIs): Detectability, Parameter Estimation and Challenges’,
Simulating Extreme Spacetime (SXS) Weekly Seminar
[Mar 2021] - ‘Numerical Relativity Surrogate model for eccentric binary black hole gravitational waveform’,
Simulating Extreme Spacetime (SXS) Weekly Seminar
[Dec 2020] - ‘Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model’,
PostDoc/Grad Student Seminar, Institute for Computational Experimental Research in Mathematics(ICERM), Brown University, USA
[November 2020]
Conference Talks
- ‘Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity’,
25th CAPRA Meeting on Radiation Reaction in General Relativity University College Dublin
[June 2022] - ‘Re-analyzing GWTC-3 events with a numerical relativity surrogate waveform model’,
APS April Meeting 2022, Session L16: Advances in Gravitational Waveform Modeling, New York
[Apr 2022] - ‘High precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles’,
Midwest Gravity Meeting 2022, University of Illinois Urbana-Champaign
[October 2021] - ‘Eccentric binary black hole surrogate models for the gravitational waveform: comparable mass, non-spinning case’,
16th Marcel Grossmann Meetings 2021, Virtual Meeting
[July 2021] - ‘A multi-mode time-domain surrogate model for gravitational wave signals from comparable to extreme mass-ratio black hole binaries’,
24th CAPRA Meeting on Radiation Reaction in General Relativity, Perimeter Institute, Virtual Meeting
[June 2021] - ‘Detectability and source characterization of intermediate mass-ratio black hole coalescences with gravitational waves’,
2238th Meeting of the American Astronomical Society (AAS), Session: Compact Mergers Observed & Compact Binary Populations through Gravitational Waves, Virtual Meeting
[June 2021] - ‘Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model’,
APS April Meeting 2021, Session Y16: Gravitational Wave Observations, Virtual Meeting
[Apr 2021] - ‘Eccentric binary black hole surrogate models for the gravitational waveform: comparable mass,nonspinning case’,
APS April Meeting 2021, Session L16: Gravitational Waveform Modeling of Compact Binaries I, Virtual Meeting
[Apr 2021] - ‘Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model’,
237th Meeting of the American Astronomical Society (AAS), Session: Compact Mergers Observed through Gravitational Waves, Virtual Meeting
[Jan 2021] - ‘Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model’,
MidWest Relativity Meeting 2020, University of Notre Dame, USA
[October 2020] - ‘Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model’,
Mathematical and Computational Approaches for Solving the Source-Free Einstein Field Equations, Advances in Computational Relativity, ICERM, Brown University, USA (Lightning Talk)
[October 2020] - ‘Numerical Relativity Surrogate model for eccentric binary black hole gravitational waveform’,
The XIII International LISA Symposium, originally planned at Glasgow, Virtual Meeting
[September 2020] - ‘Acceleration Relations in the Milky Way as Differentiators of Modified Gravity Theories’,
Cosmology from Home 2020 Conference, Virtual Meeting
[August 2020] - ‘Detectability and Parameter Estimation Accuracy for Intermediate Mass Black Holes (IMBHs) with current generation detectors’,
23rd CAPRA Meeting on Radiation Reaction in General Relativity, University of Texas Austin, Virtual Meeting
[June 2020] - ‘Testing the “no-hair” nature of binary black holes using the consistency of multipolar gravitational radiation’,
236th Meeting of the American Astronomical Society (AAS), Session: Gravitational Waves & Multi-messenger Astronomy I, Virtual Meeting, Originally scheduled to be at Madison, USA
[June 2020] - ‘Testing the “no-hair” nature of binary black holes using the consistency of multipolar gravitational radiation’,
APS April Meeting 2020, Session R05: Tests of General Relativity with Gravitational Waves II, Washington DC, USA
[April 2020] - ‘Testing Weyl gravity at galactic and extra-galactic scales’,
‘Cosmology Next Decade’ Winter School & Workshop, ICTS-TIFR, India (Student Talk)
[Jan 2019]
Conference Posters
- 'Eccentric binary black hole surrogate models for the gravitational waveform: comparable mass, nonspinning case’, Tousif Islam;
Meeting of the National Research Gropus on Gravitational Waves, Institut Henri Poincaré, Paris, France, Virtual
[March 2021] - 'Eccentric binary black hole surrogate models for the gravitational waveform: comparable mass, nonspinning case’, Tousif Islam;
Ligo-Virgo-Kagra (LVK) Collaboration March Meeting, Virtual
March 2021 - 'Eccentric binary black hole surrogate models for the gravitational waveform: comparable mass, nonspinning case’, Tousif Islam;
Gravitational waves: a new messenger to explore the universe, Institut Henri Poincaré, Paris, France, Virtual
[March 2021] - 'Detectability and Parameter Estimation Accuracy for Intermediate Mass Black Holes (IMBHs) with current generation detectors’, Tousif Islam;
39th Meeting of Astronomy Society of India (ASI), India
[Feb 2021] - Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model, Tousif Islam, Scott Field, Carl-Johan Haster & Rory Smith;
30th Meeting of Indian Association for General Relativity and Gravitation (IAGRG), IIT Gandhinagar, India
[Dec 2020] - ‘Testing the “no-hair” nature of binary black holes using the consistency of multipolar gravitational radiation’, Tousif Islam, Ajit K. Mehta, Abhirup Ghosh, Vijay Varma, P. Ajith & B. S. Sathyaprakash;
JSI Workshop : The New Faces of Black Holes, Joint Space Institute (JSI), Maryland, USA,
[Nov 2019] - ‘“No-hair” tests for binary black holes’, Tousif Islam, Abhirup Ghosh, Ajit K. Mehta & P. Ajith;
ICTS In-House Meeting, ICTS, Bengaluru, India,
[Apr 2019] - ‘A “no-hair” test for binary black holes’, Tousif Islam, Abhirup Ghosh, Ajit K. Mehta & P. Ajith;
30th Meeting of Indian Association for General Relativity and Gravitation (IAGRG), Hyderabad, India
[Jan 2019]
