INO PROJECT
Introduction
• India-based Neutrino
physics research project
1,300 meters (4,300
Nadu, India.
• This project is notable in that it is anticipated to provide a precise
measurement of neutrino mixing parameters.
• The Government will establish The India
(INO) jointly by the Department of Atomic Energy and Department of
Science and Technology
• The project is a multi
experimental particle physics
• When completed, the INO will house the world's most massive magnet,
four times larger than the 12,500
Solenoid detector at CERN in Geneva, Switzerland
Design
• The primary research instrument will consist of a 50,000 ton
magnetized iron particle physics calo
Chamber (RPC) technology as the
• The INO design is mostly based on the
not go beyond the proposal Stage. The detector was expected to start
collecting data in the year 2012. The location of INO has attracted a lot
of attention from the neutrino physics c
between INO and CERN is very close to "Magic Baseline"
which the effect of the CP phase on the measurement of
The project includes
• Construction of an underground laboratory and associated surface
facilities
• Construction of Iron calorimeter
Neutrino Observatory (INO) is a proposed particle
research project to primarily study atmospheric neutrinos
1,300 meters (4,300 ft) deep cave under Ino Peak near Theni,
This project is notable in that it is anticipated to provide a precise
measurement of neutrino mixing parameters.
The Government will establish The India-based Neutrino Observatory
(INO) jointly by the Department of Atomic Energy and Department of
Science and Technology
The project is a multi-institute collaboration and one of the biggest
particle physics projects undertaken in India
When completed, the INO will house the world's most massive magnet,
four times larger than the 12,500-tonne magnet in the Compact Muon
detector at CERN in Geneva, Switzerland
The primary research instrument will consist of a 50,000 ton
particle physics calorimeter with glass Resistive Plate
(RPC) technology as the sensor elements
The INO design is mostly based on the monolith experiment
not go beyond the proposal Stage. The detector was expected to start
collecting data in the year 2012. The location of INO has attracted a lot
of attention from the neutrino physics community as the distance
between INO and CERN is very close to "Magic Baseline" - a distance at
which the effect of the CP phase on the measurement of
Construction of an underground laboratory and associated surface
Construction of Iron calorimeter
particle
atmospheric neutrinos in a
ft) deep cave under Ino Peak near Theni, Tamil
This project is notable in that it is anticipated to provide a precise
based Neutrino Observatory
(INO) jointly by the Department of Atomic Energy and Department of
institute collaboration and one of the biggest
When completed, the INO will house the world's most massive magnet,
tonne magnet in the Compact Muon
The primary research instrument will consist of a 50,000 ton
Resistive Plate
monolith experiment that could
not go beyond the proposal Stage. The detector was expected to start
collecting data in the year 2012. The location of INO has attracted a lot
ommunity as the distance
a distance at
is minimal
Setting up of national Centre for higher energy Physics at madurai The Primary goals of the INO are the following 1. Unambiguous and more precise determination of Neutrino oscillation parameters using atmospheric neutrinos. 2. Study of matter effects through electric charge identification, that may lead to the determination of the unknown sign of one of the mass differences. 3. Study of charge-conjugation and charge parity (CP) violation in the leptonic sector as well as possible charge-conjugation, parity, timereversal(CPT) violation studies. 4. Study of Kolar events, possible identification of very-high energy neutrinos and multi-muon events.
Setting up of national Centre for higher energy Physics at madurai The Primary goals of the INO are the following 1. Unambiguous and more precise determination of Neutrino oscillation parameters using atmospheric neutrinos. 2. Study of matter effects through electric charge identification, that may lead to the determination of the unknown sign of one of the mass differences. 3. Study of charge-conjugation and charge parity (CP) violation in the leptonic sector as well as possible charge-conjugation, parity, timereversal(CPT) violation studies. 4. Study of Kolar events, possible identification of very-high energy neutrinos and multi-muon events.
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