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2004 ASTRONOMY & ASTROPHYSICS - Indian Academy of Sciences

2004 ASTRONOMY & ASTROPHYSICS - Indian Academy of Sciences

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GRAVITATION AND PARTICLE <strong>ASTROPHYSICS</strong><br />

context <strong>of</strong> structure formation and as a<br />

source <strong>of</strong> high energy cosmic rays;<br />

• Modelling <strong>of</strong> the so called Dark Energy and<br />

related issues;<br />

• Braneworld scenarios in the context <strong>of</strong> the<br />

early Universe, black hole formation, relic<br />

gravity waves and the issue <strong>of</strong> dark energy.<br />

Research related to the above problems has been<br />

carried out both at universities and in various<br />

institutes across the country. Other theoretical<br />

topics in Astroparticle Physics which are being<br />

actively pursued are:<br />

• Study <strong>of</strong> the phase-space distribution <strong>of</strong> dark<br />

matter in the Galaxy and in the Universe.<br />

• Origin <strong>of</strong> ultra high energy cosmic rays<br />

(UHECR) and issues related to probing<br />

fundamental physics beyond the Standard<br />

Model <strong>of</strong> elementary particles with UHECR.<br />

• The construction <strong>of</strong> phenomenological<br />

models <strong>of</strong> dark energy and methods aimed<br />

at reconstructing the cosmic equation <strong>of</strong><br />

state from supernova observations.<br />

• Development <strong>of</strong> higher dimensional<br />

cosmological models.<br />

• Predictions for cosmology from inflationary<br />

models, such as the spectrum and amplitude<br />

<strong>of</strong> density perturbations, and gravity waves.<br />

• Cosmological baryogenesis through<br />

leptogenesis in the Grand Unified Theories.<br />

• Study <strong>of</strong> the implications <strong>of</strong> the solar and<br />

atmospheric neutrino data for neutrino<br />

flavour oscillation phenomenology and<br />

neutrino mass hierarchy.<br />

• The study <strong>of</strong> the implications <strong>of</strong> the topdown<br />

scenario <strong>of</strong> the origin <strong>of</strong> UHECR<br />

above 10 20 eV and their testability with the<br />

up-coming large-area UHECR detectors.<br />

• The implications <strong>of</strong> UHECR for the<br />

enhanced neutrino interaction cross section<br />

predicted in some extra-dimensional models,<br />

• Cosmological implications <strong>of</strong> the possible<br />

relics <strong>of</strong> the quark-hadron phase transition in<br />

the early Universe, etc.<br />

Recommendations<br />

The committee would like to endorse the<br />

following recommendations <strong>of</strong> the Panel:<br />

1.Experimental Gravitation<br />

High priority support could be given to the<br />

existing programmes involving torsion balance<br />

experiments, in recognition <strong>of</strong> the fact that<br />

these are internationally competitive, that the<br />

programmes address significant questions <strong>of</strong><br />

fundamental import, and that these have a very<br />

high impact-to-cost ratio.<br />

2. Gravitational Waves<br />

The area <strong>of</strong> gravitational wave detection and<br />

gravitational wave physics is developing into a<br />

large team activity. Given the complexity <strong>of</strong><br />

the effort and the limited availability <strong>of</strong> trained<br />

manpower, on the one hand, and the<br />

improved communications and the long reach<br />

<strong>of</strong> the internet on the other, it <strong>of</strong>fers the<br />

interested <strong>Indian</strong> scientists an alternative way<br />

to participate in an exciting endeavour. Most<br />

<strong>of</strong> the experiments <strong>of</strong>fer the possibility to<br />

participate in the science collaboration against<br />

specific deliverables.<br />

Data analysis has been recognized as a key<br />

aspect in searching for gravitational waves.<br />

Experience in handling large volumes <strong>of</strong> data<br />

and the development <strong>of</strong> sophisticated analysis<br />

algorithms will therefore play a vital role in the<br />

eventual success <strong>of</strong> gravitational wave<br />

detection. Prior to these instruments becoming<br />

fully operational, data analysis is also an<br />

106

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