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SOME ASPECTS OF STRANGE MATTER : STARS AND STRANGELETS

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2. Changing airspace environment in Eastern Himalayas. 3. Children's science resource centre ... Eastern Himalayas. Radio Environment. Chemical, Physical, and ... – PowerPoint PPT presentation

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Title: SOME ASPECTS OF STRANGE MATTER : STARS AND STRANGELETS


1
Centre for Astroparticle Physics and Space
Sciences A National Facility at Bose
Institute (A project under IRHPA
Scheme) Sibaji Raha Bose Institute Kolkata
2

Acharya J.C. Bose (1858 1937)
3
Thus the lines of physics, of physiology and
psychology converge and meet. And here will
assemble those who would seek oneness amidst the
manifold Acharya J.C.Bose
4
Genesis Mission
  • Drawn by Nationalist zeal,
  • Missionary vision,
  • Faith in the ability of
    Indians
  • Not merely a laboratory but a temple
  • 1896 visit to Royal Institution, London
  • Took firm roots of the Idea
  • 1915 Retirement from Education Service
  • 1917 Bose Institute was Founded

5
And in this country through millenniums, there
always have been some who, beyond the immediate
and absorbing prize of the hour, sought for the
realization of the highest ideal of life not
through passive renunciation, but through active
struggle
6
The advancement of science is the principal
object of the Institute, and also the diffusion
of knowledge
7
In this institutethe claim of art has not been
forgotten, for the artist has been working with
us, from foundation to pinnacle and from floor to
ceiling of this very hall.
8
And beyond the arch, the laboratory merges
imperceptibly into the garden which is true
laboratory for the study of life. There the
creepers, the plants and trees are played upon by
natural environment, sunlight and wind and where
they will be subjected to chromatic action of
different lights, to invisible rays, to
electrified ground or thunder-charged atmosphere.
9
India is drawn into the vortex of international
competition. She has to become efficient in every
way through spread of education, through
performance of civic duties and responsibilities,
through activities both industrial and
commercial. Neglect of these essentials of
national duty will imperil her very existence.
Acharya J.C.Bose
10
  • Origin
  • In-house expertise Need for consolidation
  • Darjeeling Campus Location Opportunities
  • (a) Cosmic Ray
  • (b) Atmospheric Chemistry
  • (c) Radiometric studies

11
  • Four major programmes
  • 1. Cosmic ray studies at high altitude
  • 2. Changing airspace environment in Eastern
    Himalayas
  • 3. Childrens science resource centre
  • 4. Manpower development training programmes

12
Cosmic Ray studies
13
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14
Electrons electric cherge - EM force
Photon Quarks - Colour Charge - Strong force
Gluon
15
Quark three colours - Red , Blue , Green
Gluons eight - red anti-blue and other
combinations Mesons quarkantiquark
colouranticolour WHITE Baryons three quarks
redbluegreen - WHITE
16
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18
  • H- matter ? P.T. ? Q matter
  • SQM ? Ground state of matter
  • First idea Bodmer (1971)
  • Resurrected Witten (1984)
  • Stable SQM Conflict with
  • experience ????
  • 2-flavour energy gt 3-flavour
  • Lowering due to extra Fermi well
  • Stable QM ? 3-flavour matter
  • Stable SQM ? significant amount
  • s quarks
  • For nuclei ? high order of weak
  • interaction to convert u d to s

19
  • SQM Strangelet Search
  • SQM
  • Early universe quark-hadron phase transition
  • Quark nugget ? MACHO
  • 2. Compact stars (Core of Neutron Stars or Quark
    Stars)
  • Strangelets
  • Heavy Ion Collision
  • Short time
  • Much smaller size A 10-20
  • Stability Problem at high temperature
  • 2. Cosmic Ray events
  • Collision of Strange stars or other
    strange objects Shower

20
Detection of strangelets ? Propagation mechanism
of strangelets ? How far can it travel through
atmosphere ? How does it interact with atmosphere
? Important observations ? Stability of strange
matter ? Small positive charge ? massive s
quark ? Z/A ?? 1
21
  • Remarks
  • ? Detection of strangelets Passive
    detectors
  • ? Active detectors Air shower studies in
    collaboration

22
Study of Changing airspace environment in
Eastern Himalayas
23
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24
  • Indo-Gangetic plane
  • ? Agricultural as well as Industrial
    activity
  • ? Source of atmospheric pollutants
  • ? Vulnerable place from changing
    environment
  • Himalaya is subject to
  • (a) emissions from IGP regions
  • (b) pollutants transported from long
    distances
  • Himalaya Unique place to monitor airspace
  • environment

25
  • Eastern Himalaya wet with rich forest cover
    and
  • lesser
    population
  • Western Himalaya dry, scanty forest cover and
  • high
    population
  • Monitoring stations
  • Mostly in western Himalaya

26
Eastern Himalaya Monitoring stations
Pyramid Station 5034 meters
Sandakphu 4200 meters
Kathmandu ICIMOD-UCSD Station
Darjeeling 2500 meters
North Bengal University, Siliguri
27
Physical Environment
Chemical Environment
Monitoring of trans-boundary pollutants
H2O mm waves O3, CO, NOx, SO2 Trace
Species Aerosols Scattering/ Absorbing
Met Data
3-D Trajectories
Eastern Himalayas
23.8 GHz (Water Vapour) 31.4 GHz (Liquid
Water) Distrometers (DSD)
Radio Environment
Emission Inventories
Air Pollutant Dispersal 3-D Chemical Modeling
Chemical, Physical, and Radio Mapping of the
region
28
  • Project II-AI (IITM)
  • Atmospheric Chemistry-Aerosol-Climate Interaction
  • Objectives  To monitor physical, chemical and
    optical characteristics of aerosols under
    different air mass situations   To
    investigate the role of radiative forcing of
    aerosols in the climate system using experimental
    observations and model computations  To assess
    the influence of terrain / meteorological
    conditions on aerosol parameters

29
  • Project II-AII (NPL)
  • Chemical behaviour of aerosols, greenhouse gases,
    trajectory analysis and impact of particulate
    matter loading on human health
  • Objectives  To monitor greenhouse gases and
    pollutants for understanding trans-boundary flow
      To investigate the chemical characteristics
    of aerosols and back trajectory analysis for
    source apportionment  To assess the impacts of
    particulate matter loading on human health

30
  • Expected outcome
  • Mass-size distribution of aerosols
  • Monthly, seasonal and diurnal variation of
    aerosol, trace and green house gas, partulate
    matter concentrations
  • Influence of meteorological parameters on air
    pollutants
  • Chemical composition of precipitation and
    aerosols
  • Impacts of aerosol loading on atmospheric
    radiative forcing
  • Trans-boundary flow of pollutants
  • Impact of pollutants on regional climate
  • Relation between atmospheric pollution loading
    and human health hazards

31
  • Various measurements, as mentioned below, will be
    undertaken. Continuous monitoring will take place
    at the Darjeeling site and measurements at
    Siliguri and Sandakphu will be made in campaign
    mode. These measurements at varying altitudes
    will provide some information about height
    profiles.
  • Atmospheric surface ozone
  • Columnar ozone (indirect)
  • Radiation measurements including UV radiation
  • Trace and Green House gases (NO2, SO2, NOx, SOx,
    CO, CO2, CH4 and N2O)
  • Physical and chemical characteristics of Aerosols
    (Scattering/absorbing) including carbonaceous
    aerosols
  • Precipitation chemistry
  • Biogenic organic particulate matter
  • Meteorological Parameters

32
Project II-B
  • STUDIES ON ATMOSPHERIC WATER VAPOUR AND CLOUD
    LIQUID WATER USING DUAL FREQUENCY RADIOMETER AND
    RELATED RAIN/FOG ENVIRONMENT AT THE HIGH ALTITUDE
    STATION AT DARJEELING

33
  • IWV and LWP with a dual-frequency radiometer
    operating at 23.8 and 31.4 GHz.
  • Rain attenuation over earth-space paths by
    receiving satellite signals at Ku/Ka bands.
  • Rain rate with an optical rain-gauge
  • Rain drop size distribution with a Disdrometer.
  • The following studies are proposed with the
    above-mentioned experimental measurements
  • Variation of atmospheric water vapour, cloud
    liquid water content with time season, season,
    and their relationship with surface weather
    parameters, such as, temperature, relative
    humidity etc.
  • Modelling of cloud liquid water content and
    comparison of the derived model with the
    available global models.
  • To indicate the inter-relationship between IWP
    and LWP
  • To relate the rain attenuation over earth-space
    paths with the rain rate at the receiving site of
    satellite signal that will give an integrated
    picture of rain rate over the satellite path.
  • To relate rain DSD with radiometric observations
    during rain. Also, rain DSD will provide liquid
    water content in rain, which may be related with
    IWV and LWP. These integrated measurements will
    be used to study the interrelation among cloud
    liquid water, water vapour and rain at Darjeeling

34
  • Childrens Science Resource Centre

35
  • 1. Formation of science clubs in schools
  • 2. Train them to record local meteorological
    data
  • 3. Once in a month meeting, recording of data
    taken
  • by students in the central data base
  • 4. Train some of the interested students for
    cosmic ray
  • experiments
  • 5. Introductory level lectures by scientists

36

Manpower development
37
  • Workshops and summer schools on various
  • aspects of the
  • cosmic ray physics
  • Instrumentation
  • Environmental science
  • Weather modeling studies
  • Numerical simulation
  • with hands-on training
  • Aimed at Masters level and beginning doctoral
  • students

38
Thank You
39
  • Cosmic rays
  • Cosmic rays are high energy charged particles,
    originating in outer space, that travel at nearly
    the speed of light and strike the Earth from all
    directions.
  • Cosmic ray ions at the top of the energy
    range produce in the atmosphere showers of many
    millions of fragments, covering many acres, and
    their more energetic fragments register even in
    deep mines, a mile underground. back

40
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