IndIGOIndian Initiative in Gravitational-wave Observations

Application for GWIC Membership

Bala IyerChair, IndIGO Consortium Council

Raman Research Institute, Bangalore

GWIC Meeting, Cardiff, 10 July 2011

Gravitational wave legacy in India• Internationally recognized Indian contribution over two decades to

the global effort for detecting GW on two significant fronts • Seminal contributions to source modeling at RRI [Bala Iyer] and to GW data analysis at IUCAA [Sanjeev Dhurandhar]• RRI: Indo-French collaboration for two decades to compute high accuracy

waveforms for in-spiraling compact binaries from which the GW templates used in LIGO and Virgo are constructed. Cardiff collaboration on improved detection templates, parameter estimation, implications for Astrophyscs and cosmology

• IUCAA: Designing efficient data analysis algorithms involving advanced mathematical concepts.. Notable contributions include the search for binary in-spirals, hierarchical methods, coherent search with a network of detectors and the radiometric search for stochastic gravitational waves.

• IUCAA: Tarun Souradeep with expertise in CMB data & Planck creates bridge between CMB and GW data analysis challenges : stochastic GW background maps

• IUCAA has collaborated with most international GW detector groups and has been a member of the LIGO Scientific Collaboration (LSC) for a decade.

Multi-Institutional,Multi-disciplinary Consortium(2009)

1. CMI, Chennai2. Delhi University3. IISER Kolkata4. IISER Trivandrum5. IIT Madras (EE)6. IIT Kanpur (EE)7. IUCAA, Pune8. RRCAT, Indore9. TIFR, Mumbai10. IPR, Bhatt

Others• RRI• Jamia Milia Islamia• Tezpur Univ

Nodal Institutions

IndIGO: The goals

• Provide a common umbrella to initiate and expand GW related experimental activity and train new technically skilled manpower

• Seek pan-Indian consolidated IndIGO membership in LIGO Scientific Collaboration (LSC) for participation in Advanced LIGO.

• Create a Tier-2 data centre in IUCAA for LIGO Scientific Collaboration Deliverables and as a LSC Resource

• Start collaborative work on joint projects under the IUSSTF Indo-US IUCAA-Caltech joint Centre at IUCAA

• Indo-Jap project “Coherent multi-detector gravitational wave search using LCGT and advanced interferometers”

• Explore the Roadmap for EGO-IndIGO collaboration on GW and a possible MOU (Meeting on Nov 1-2 ,2011 at IUCAA)

• Explore Indian participation in LISA and space based GW detectors in the future ( ASTROD 5 meeting on July 14 – 16, 2012 at RRI)

The IndIGO Consortium

Data Analysis & Theory

1. Sanjeev Dhurandhar IUCAA2. Bala Iyer RRI3. Tarun Souradeep IUCAA4. Anand Sengupta Delhi University 5. Archana Pai IISER, Thiruvananthapuram6. Sanjit Mitra JPL , IUCAA7. K G Arun Chennai Math. Inst., Chennai8. Rajesh Nayak IISER, Kolkata9. A. Gopakumar TIFR, Mumbai 10. T R Seshadri Delhi University 11. Patrick Dasgupta Delhi University12. Sanjay Jhingan Jamila Milia Islamia, Delhi13. L. Sriramkumar, Phys., IIT M14. Bhim P. Sarma Tezpur Univ . 15. Sanjay Sahay BITS, Goa16. P Ajith Caltech , USA17. Sukanta Bose, Wash. U., USA18. B. S. Sathyaprakash Cardiff University, UK19. Soumya Mohanty UTB, Brownsville , USA20. Badri Krishnan Max Planck AEI, Germany

Instrumentation & Experiment

1. C. S. Unnikrishnan TIFR, Mumbai2. G Rajalakshmi TIFR, Mumbai3. P.K. Gupta RRCAT, Indore 4. Sendhil Raja RRCAT, Indore5. S.K. Shukla RRCAT, Indore6. Raja Rao ex RRCAT, Consultant 7. Anil Prabhakar, EE, IIT M8. Pradeep Kumar, EE, IIT K9. Ajai Kumar IPR, Bhatt10. S.K. Bhatt IPR, Bhatt 11. Ranjan Gupta IUCAA, Pune12. Bhal Chandra Joshi NCRA, Pune13. Rijuparna Chakraborty, Cote d’Azur, Grasse14. Rana Adhikari Caltech, USA 15. Suresh Doravari Caltech, USA 16. Biplab Bhawal (ex LIGO)

IndIGO Council1. Bala Iyer ( Chair) RRI,

Bangalore 2. Sanjeev Dhurandhar (Science) IUCAA, Pune 3. C. S. Unnikrishnan (Experiment) TIFR, Mumbai4. Tarun Souradeep (Spokesperson) IUCAA, Pune

Committees: National Steering Committee:Kailash Rustagi (IIT, Mumbai) [Chair]Bala Iyer (RRI) [Coordinator]Sanjeev Dhurandhar (IUCAA) [Co-Coordinator]D.D. Bhawalkar (Quantalase, Indore)[Advisor]P.K. Kaw (IPR)Ajit Kembhavi (IUCAA) P.D. Gupta (RRCAT)J.V. Narlikar (IUCAA)G. Srinivasan

International Advisory Committee

Abhay Ashtekar (Penn SU)[ Chair]Rana Adhikari (LIGO, Caltech, USA)David Blair (AIGO, UWA, Australia)Adalberto Giazotto (Virgo, Italy)P.D. Gupta (Director, RRCAT, India)James Hough (GEO ; Glasgow, UK)[GWIC Chair]Kazuaki Kuroda (LCGT, Japan)Harald Lueck (GEO, Germany)Nary Man (Virgo, France)Jay Marx (LIGO, Director, USA)David McClelland (AIGO, ANU, Australia)Jesper Munch (Chair, ACIGA, Australia)B.S. Sathyaprakash (GEO, Cardiff Univ, UK)Bernard F. Schutz (GEO, Director AEI, Germany)Jean-Yves Vinet (Virgo, France)Stan Whitcomb (LIGO, Caltech, USA)

IndIGO Advisory Structure

Program Management Committee:C S Unnikrishnan (TIFR, Mumbai), [Chair]Bala R Iyer (RRI, Bangalore), [Coordinator]Sanjeev Dhurandhar (IUCAA, Pune) [Co-cordinator]Tarun Souradeep (IUCAA, Pune)Bhal Chandra Joshi (NCRA, Pune)P Sreekumar (ISAC, Bangalore)P K Gupta (RRCAT, Indore)S K Shukla (RRCAT, Indore)Sendhil Raja (RRCAT, Indore)]

LSC Collaboration from India• Aug 2000 - 2010 MOU between IUCAA (Sanjeev Dhurandhar) and LIGO (LSC)• Projects carried out under LIGO Scientific Collaboration (LSC) - Hierarchical GW Search for inspiralling compact binaries as part of inspiral

group of LSC with Anand Sengupta and the inspiral group -Radiometric search for GW stochastic background as part of stochastic

group of LSC with Sanjit Mitra, Tarun Souradeep, IUCAA - Radiometric search for Pulsars as part of continuous wave group of LSC

with Himan Mukhopadhyay, Badri Krishnan, AEI and John Whelan, AEI -All sky and all frequency search with Badri Krishnan, AEI• The most recent work in progress is on the fast transform for continuous

sources which is based on group theoretic methods.

• Proposal in preparation to consolidate IUCAA participation in LSC to IndIGO participation in Advanced LIGO with GW 2 tier Data Center

High precision experimental expertise in India• TIFR [C.S. Unnikrishnan] : High precision experiments and tests of weak forces

– Test gravitation using most sensitive torsional balances and optical sensors.– Techniques related to precision laser spectroscopy, electronic locking, stabilization.

– G.Rajalakshmi (IIA TIFR, 3m prototype); – Suresh Doravari (IIA LIGO, Caltech expt./AdvLIGO)

• IITM [Anil Prabhakar] and IITK [Pradeep Kumar] (EE depts)– Photonics, Fiber optics and communications– Characterization and testing of optical components and instruments for use in India..

• RRCAT – [S.K. Shukla on INDUS, A.S. Raja Rao (exRRCAT)] --UHV– [Sendhil Raja, P.K. Gupta] - Optical system design, laser based

instrumentation, optical metrology, Large aperture optics, diffractive optics, micro-optic system design.

– [Rijuparna Chakraborty, France LIGO/EGO pdf?] Adaptive Optics….

Large experiment expertise in India• RRCAT….• IPR [S.B. Bhatt on Aditya and Ajai Kumar] - UHV experience, Lasers… Support role in large volume UHV system, Control systems,….• Groups at BARC and RRCAT : involved in LHC

– providing a variety of components and subsystems like precision magnet positioning stand jacks, superconducting correcting magnets, quench heater protection supplies and skilled manpower support for magnetic tests and measurement and help in commissioning LHC subsystems.

• Teams at Electronics & Instrumentation Groups at BARC (may be interested in large instrumentation projects in XII plan)• Groups at ISRO,…….• Over the last two years contacts have been made with

members of the above groups to explore their participation in the proposed experimental initiatives should a national mega project on GW be funded in India.

IndIGO: The Aspirations

• Set up a major experimental initiative in GW astronomy MOU with ACIGA to collaborate on GW AstronomyTwo Alternatives depending on the Australian decisionPartner in LIGO-Australia

– Indian partnership at 15% of Australian cost with full data rights

Another Developing possibility…LIGO-India– Letter from LIGO Labs with offer of LIGO-India and Requirement Document

IndIGO Consortium has worked towards getting these alternatives discussed among other National Mega Projects in the coming Five year plan in India. For the latter alternative, seeking National Flagship Mega Project status to ensure requirements from the LIGO-Lab can be met in time to seek the required NSF and US govt approvals.

LIGO-India: Why is it a good idea?• Geographical relocation Strategic for GW astronomy

– Increased event rates (x2-4) by coherent analysis – Improved duty cycle– Improved Detection confidence– Improved Sky Coverage– Improved Source Location required for multi-messenger astronomy– Improved Determination of the two GW polarizations

• Potentially large Indian science user community in the future– Indian demographics: youth dominated – need challenges– Improved UG education system will produce a larger number of students

with aspirations looking for frontline research opportunity at home.• Substantial data analysis trained faculty exists in India and

Large Data Analysis Center Facilities are being planned

IndIGO 3m Prototype DetectorFunded by TIFR Mumbai on campus (2010)PI: C. S.Unnikrishnan ( INR 3.5cr ~.7 M$

$) Goals of the TIFR 3-m prototype interferometer (to be operational in 2014):

1) Research and Training platform with all the features of the advanced LIGO-like detectors, scaled down to displacement sensitivity around 10-18 m, above 200 Hz.

2) The Indian research platform for features like signal recycling, DC read-out, and most importantly the use of squeezed light and noise reduction (last phase).

3) Instrument for studies on short range gravity and QED force, especially a measurement of the Casimir force in the range 10 -100 microns where no previous measurements exist (Rajalakshmi and Unnikrishnan, Class, Quant. Grav. 27, 215007 (2010).

Frequency (Hz)

1 10 100 1000

10-20

10-19

10-18

10-17

10-16

10-15

10-14

Shot noise

Seismic (best and worst case, dashed)

( / )l m Hz

10000Signal recycling + Squeezing

SQL

Sketch of expected sensitivity for 3-m prototype

Best case total

suspension noise

OldLIGO

Indo-US centre for Gravitational Physics and Astronomy @ IUCAA

• Centre of Indo-US Science and Technology Forum (IUSSTF)

• Exchange program to fund mutual visits and facilitate interaction.

• Nodal centres: IUCAA , India & Caltech, USA.

• Institutions:

Indian: IUCAA, TIFR, IISER, DU, CMI - PI: Tarun Souradeep USA: Caltech, WSU - PI: Rana Adhikari

APPROVED for funding (Dec 2010)

Participation in LSC during Advanced LIGOProposed Data Analysis activities of the IndIGO Consortium

•Principal Leads: K.G. Arun, R.Nayak, A. Pai, A. Sengupta, S. Mitra

• Participants: S. Dhurandhar, T.Souradeep, B. R. Iyer, C.K. Mishra, M.K. Harris,….

• Institutions: CMI, IUCAA, IISER (Kolkata), IISER (Tvm), Univ Delhi

•Projects• Multi-detector Coherent veto• Tests of GR and alternative theories of gravity• Stochastic Gravitational wave background analysis

• IndIGO Data Center

Primary Science: Online Coherent search for GW signal from binary mergers using data from global detector network

Coherent 2-4 x event rate (40 80-160 /yr for NS-NS) Role of IndIGO data centre

Large Tier-2 data/compute centre for archival of GW data and analysis Bring together data-analysts within the Indian gravity wave community. Puts IndIGO on the global map for international collaboration with LIGO

Scientific Collaboration. Facility for LSC as part of IndIGO participation. Large University sector participation via IUCAA

• 200 Tflops peak capability (by 2014) • Storage: 4x100TB per year per interferometer.• Network: gigabit+ backbone, National Knowledge Network• Gigabit dedicated link to LIGO lab Caltech

• 20 Tf 200 Tb funded IUCAA : ready Mid 2012

IndIGO Data Centre @ IUCAA Anand Sengupta, DU, IndIGO

Concluding Remarks..• Over two decades India has been involved in quality GW research and been a

part of the International GW community

• Since 2009 Indian aspirations involve participation in a major GW experiment eventually leading to a GW detector in India

• The Indian Aspirations in GW research are represented by the IndIGO Consortium

• With help from the International GW community IndIGO has made significant progress to integrate into the GWIC plans towards the setting up of a GW detector network

• IndIGO has concrete plans as outlined in the presentation to increase participation in GW research in the coming years.

• By becoming a member of GWIC, IndIGO can contribute more effectively in the future towards the GWIC agenda to detect GW leading on to Gravitational wave Astronomy..

THANK YOU

GW Research in India (Pre IndIGO:1990 -2009)

• Regular International Collaboration with GW groups in Australia, France, Germany, UK, Japan since 1990

• September 1990: Interferometric Gravity wave Detector: Phase I: Developmental work and Experiments, A proposal by

IUCAA, Pune [S.V. Dhurandhar, N.K. Dadhich, J.V. Narlikar, S.N. Tandon] and CAT, Indore [P.K. Gupta, A.S. Raja Rao, D.D. Bhawalkar] 1.25 cr, Staffing 21 Phase II: 100 m Detector : 13 crores, Staffing 51

• December 1995: Design of the Vacuum system for AIGO 500 ( CAT/95-16, Indore) [A.S. Raja Rao]• International GW Collaborative Projects• 1991, 1993, 1994, 1995 IUCAA- UWA Informal Collaboration [Sanjeev Dhurandhar (IUCAA) and David Blair (UWA) and David McClelland (ANU)]• 1995 -1998 Indo-French Project: 1010-1 Modelling of non-linear effects in high power optical cavities of laser

interferometric gravitational wave detectors [S.V. Dhurandhar (IUCAA) and Jean-Yves Vinet (Laboratoire de l'Accelerateur, Orsay]• 2000 – 2004 Indo-French Project: 2204-1

Gravitational wave data analysis for laser interferometer space antenna[S.V. Dhurandhar (IUCAA) and Jean-Yves Vinet (Observatoire de la Cote d'Azur, Nice)]

• 2003 – 2007 Indo-French Project: 2904-1 Gravitational Waves from Neutron Star Binaries, [Bala Iyer (RRI) and Luc Blanchet (IAP) ]

• 2006 - 2009 Indo-French Project: 3504-1 - Physical and mathematical modeling of LISA mission [S.V. Dhurandhar (IUCAA) and Bertrand Chauvineau (Observatoire de la Côte d’Azur, Nice)]

• 2006 - 2009 Indo-French Project: 3504-3 - Systematic effects in CMB of ESA’s Satellite “PLANCK”[Tarun Souradeep (IUCAA) and François R. Bouchet (Institut d’Astrophysique de Paris)]

• 2010 - 2013 Indo-French Project: 4204-2 High accuracy gravitational waves from black hole binaries [Bala Iyer (RRI) with Luc Blanchet (IAP), Guillaume Faye (IAP) ]

• 2006 - 2011 DST-JSPS Indo-Japanese Collaboration Coincident vs Coherent multi-detector strategies for inspiralling binaries [Sanjeev Dhurandhar (IUCAA), Nobuyuki Kanda (Osaka University) and Hideyuki Tagoshi, (Osaka University)]

IndIGO Consortium – Milestones

• Late 2007 : ICGC2007 @IUCAA: Rana Adhikari’s visit & discussions• 2009:

– Australia-India S&T collaboration Establishing Australia-India collaboration in GW Astronomy

– IndIGO Consortium: Reunion meeting IUCAA – GW Astronomy Roadmap for India;

• 2009-2011: – Meetings at Kochi, Pune, Shanghai, Perth, Delhi to Define, Reorient and Respond to the Global (GWIC) strategies

for setting up the International GW Network. – Bring together scattered Indian Experimental Expertise;

Individuals & Institutions• March 2011: IndIGO-I Proposal: Participation in LIGO-Australia• May 2011+: LIGO-India..

Indian Gravitational wave community strengths

• Very good students and post-docs produced who have become..

* Leaders in GW research abroad [Sathyaprakash, Bose, Mohanty] (3) *New faculty at premier institutions in India (6) [Gopakumar, Archana Pai, Rajesh Nayak, Anand Sengupta, K.G. Arun, Sanjit Mitra, P. Ajith?]

• Strong Indian presence in GW Astronomy in the Global detector network where broad international collaboration is the norm

relatively easy to get well trained researchers back • Close interactions with the very supportive International

community as reflected in the International Advisory committee of IndIGO – Chair: Abhay Ashtekar

• LIGO-Lab participation in IndIGO schools, commitment to training and assisting in high end technology tasks related to GW experiments should LIGO-India come about.

LIGO-India: Indian Requirements • Indian contribution in infrastructure : Site Vacuum systemRelated ControlsData centre Trained manpower for installation and

commissioning Trained manpower for LIGO-India operations for 10

years

Requirements:

• Low seismicity • Low human generated noise• Air connectivity• Proximity to Academic institutions, labs, industry preferred, …

LIGO-India: … the challenges

Indian Site

Preliminary exploration: IISc new campus & adjoining campuses near Chitra Durga

• low seismicity• Solid rock base• 1hr from International airport• Bangalore: science & tech hub• National science facilities complex plans power and

other infrastructure availability, ….

Manpower generation for sustenance of LIGO-India : Preliminary Plans & exploration

• Since Advanced LIGO will have a lead time, participants will be identified who will be deputed to take part in the commissioning of Advanced LIGO and later bring in the experience to LIGO-India. They will start building groups with associated training program.

• Successful IndIGO Summer internships in International labs underwayo High UG applications 30/40 each year from IIT, IISER, NISERS,..o 2 summers, 10 students, 1 starting PhD at LIGO-MITo Plan to extend to participating National labs to generate more experimenters

• IndIGO schools are planned annually to expose students to emerging opportunity in GW scienceo 1st IndIGO school in Dec 2010 in Delhi Univ. (thru IUCAA)

• Post graduate school specialization courses , or moreJayant Narlikar: “Since sophisticated technology is involved IndIGO should

like ISRO or BARC training school set up a program where after successful completion of the training, jobs are assured.”

Courtesy: Steven Fairhurst

LIGO-India: … the opportunityStrategic Geographical relocation

Polarization info

Uniformity of Sky coverage

Courtesy: S. Klimenko and G. Vedovato

LIGO-India: … the opportunity

Strategic Geographical relocation

Source localization error

5-15 degrees to ~degree !!!

Courtesy: S. Klimenko and G. Vedovato

LIGO-India: … the opportunity

Strategic Geographical relocation- the science gain

Sky coverage: Synthesized Network beam(antenna power)

Courtesy: Bernard Schutz

LIGO-India: … the opportunity

Strategic Geographical relocation- the science gain

Sky coverage: ‘reach’ /sensitivity in different directions

Courtesy: Bernard Schutz

Network HHLV HILV AHLV

Mean horizon distance

1.74 1.57 1.69

Detection Volume

8.98 8.77 8.93

Volume Filling factor

41.00% 54.00% 44.00%

Triple Detection Rate(80%)

4.86 5.95 6.06

Triple Detection Rate(95%)

7.81 8.13 8.28

Sky Coverage: 81%

47.30% 79.00% 53.50%

Directional Precision

0.66 2.02 3.01

Strategic geographical relocation comparison

Courtesy Bernard Schutz

Vacuum tanksDetector

Laser table

Vibration isolationschematic

All mirros and beamsplitters are suspended from 4-stage vib. isolators

3.5 meters

0.8 mF-P cavityPower recycling

Sensing &Control

60 cm

180 cm

Mirror

6 m6 m

The TIFR 3-m prototype detector

15 cm dia. mirrors (3 kg), 1 W NPRO laser, 2 stage passive pre-isolation, 10-9 mbar UHV

RRCAT (Next Plan period): Advanced Interferometry (Narrow line width Frequency Stabilised laser development)

The laser will be an injection seeded Nd;YAG or Yb:Silica fiber laser locked to a stabilized reference cavity. The target would be to demonstrate a laser with 1W output and sub-kHz line width and few Hz stability. Scaling up of the power to 10W will be done as the next step.

RRCAT: Advanced Interferometry (Ultraflat Components development)

Development of Ultraflat Optical components such as mirrors for GWD will require augmenting the existing facility with an ion beam figuring system for final correction of the polished optics to /500 or better.

Photonics @ IIT-Madras11 faculty members (8 in EE, 3 in Physics)10 M. Tech scholars in EE (Photonics)20+ research scholars (M.S. and Ph.D.)

Research specializations➲ Optical communications➲ Fiber lasers➲ Diffractive optical elements➲ Silicon photonics, plasmonics➲ Nonlinear and quantum optics➲ Metrology and instrumentation

Strong industry partnerships

IIT-M, IIT-K participation in LIGO

Photonics research

➲ Squeezed state detection➲ High power lasers➲ Diffractive optics➲ Silicon photonics

Manpower training➲ 2-3 research fellows each year➲ Sabbatical, or on lien, with LIGO-India ➲ Up to 20% of regular faculty time

Possible IndIGO Contributions to 3G Detectors (ET)

•Development of the lasers systems, investigate emerging laser technologies such as fiber lasers for developing a suitable laser for 3rd generation detector.•Develop squeezed light sources suitable for use in GWD.•Design and development of diffractive optical components for generating higher order Laguerre-Gauss mode laser beams.•Investigate instabilities due to quantum back action on cavity mirrors.•Development of high flatness fused silica/silicon optics and develop fabrication and metrology techniques.

Possible IndIGO Contributions to 3G Detectors (ET)

•Design and development of high power optical coating for the detector optics.•Develop techniques for absorption measurement of high purity Si as a possible optical substrate at 1.5 micron laser wavelength.•Develop high accuracy wavefront sensing and laser scanning based thermal compensation of cavity mirrors.•Investigate possible techniques to cool the detector mirrors in a non contact way (laser cooling of Yb doped glasses have been demonstrated)