day 2 polarisation of the cmb
play

Day 2: Polarisation of the CMB Eiichiro Komatsu [Max Planck - PowerPoint PPT Presentation

Jul 02, 2023 •27 likes •1.01k views

Lecture notes: https://wwwmpa.mpa-garching.mpg.de/~komatsu/lectures--reviews.html Day 2: Polarisation of the CMB Eiichiro Komatsu [Max Planck Institute for Astrophysics] University of Amsterdam March 5, 2020 How do we measure gravitational

  1. Lecture notes: https://wwwmpa.mpa-garching.mpg.de/~komatsu/lectures--reviews.html Day 2: Polarisation of the CMB Eiichiro Komatsu [Max Planck Institute for Astrophysics] University of Amsterdam March 5, 2020

  2. How do we measure gravitational waves?

  3. Measuring GW • GW changes distances between two points X d ` 2 = d x 2 = � ij dx i dx j ij d ` 2 = X ( � ij + h ij ) dx i dx j ij

  4. Laser Interferometer Mirror Mirror detector No signal

  5. Laser Interferometer Mirror Mirror detector Signal!

  6. LIGO detected GW from a binary blackholes, with a frequency of ~100 Hz = the wavelength of thousands of kilometres But, the primordial GW affecting the CMB has a frequency of 10 –18 Hz = the wavelength of billions of light-years !! How do we find it?

  7. Detecting GW by CMB Isotropic electro-magnetic fields

  8. <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> Detecting GW by CMB GW propagating in isotropic electro-magnetic fields h + h × ij ij

  9. <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="NwsD1SgjkJfMeVFacsNc7+DBIRA=">AB+HicbVBNS8NAEJ34WetHox69BIvgqSQi6LHoxWMF+wFtDZvtpl272YTdiVBDfokXD4p49ad489+4bXPQ1gcDj/dmJkXJIJrdN1va2V1bX1js7RV3t7Z3avY+wctHaeKsiaNRaw6AdFMcMmayFGwTqIYiQLB2sH4euq3H5nSPJZ3OElYPyJDyUNOCRrJtysjP+MP+X3WQx4xnft21a25MzjLxCtIFQo0fPurN4hpGjGJVBCtu56bYD8jCjkVLC/3Us0SQsdkyLqGSmK29LPZ4blzYpSBE8bKlERnpv6eyEik9SQKTGdEcKQXvan4n9dNMbzsZ1wmKTJ54vCVDgYO9MUnAFXjKYGEKo4uZWh46IhRNVmUTgrf48jJpndU8t+bdnlfrV0UcJTiCYzgFDy6gDjfQgCZQSOEZXuHNerJerHfrY96YhUzh/AH1ucPjLyTpw=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> <latexit sha1_base64="+b4698YGkh1ezVXsa0LwhPMRkAM=">AB8XicbVDLSgNBEOz1GeMr6tHLYBAEIeyKoMegF48RzAOTNcxOZpMxs7PLTK8Qlv0Lx4U8erfePNvnDwOmljQUFR1090VJFIYdN1vZ2l5ZXVtvbBR3Nza3tkt7e03TJxqxuslrFuBdRwKRSvo0DJW4nmNAokbwbD67HfOLaiFjd4SjhfkT7SoSCUbTS/aCbicf8ITvNu6WyW3EnIvEm5EyzFDrlr46vZilEVfIJDWm7bkJ+hnVKJjkebGTGp5QNqR93rZU0YgbP5tcnJNjq/RIGtbCslE/T2R0ciYURTYzojiwMx7Y/E/r51ieOlnQiUpcsWmi8JUEozJ+H3SE5ozlCNLKNPC3krYgGrK0IZUtCF48y8vksZxXMr3u15uXo1i6MAh3AEJ+DBVThBmpQBwYKnuEV3hzjvDjvzse0dcmZzRzAHzifP7yOkPE=</latexit> Detecting GW by CMB Space is stretched => Wavelength of light is also stretched d l o c h hot o t cold cold h o t hot d l o c h + h × ij ij

Recommend

Top polarisation at colliders Top polarisation: what physics can it probe Probes of the top

Top polarisation at colliders Top polarisation: what physics can it probe Probes of the top

Top polarisation at colliders. Rohini M. Godbole Top polarisation at colliders Top polarisation: what physics can it probe Probes of the top polarisation and effects of anomalous coupling on them. Example of use of angular

788 views • 62 slides
Lecture 5 - Polarisation (continued) - Gravitational waves and their imprints on the CMB The

Lecture 5 - Polarisation (continued) - Gravitational waves and their imprints on the CMB The

Lecture 5 - Polarisation (continued) - Gravitational waves and their imprints on the CMB The Single Most Important Things You Need to Remeber Polarisation is generated by the local quadrupole temperature anisotropy , which is proportional to

723 views • 45 slides
Lecture 4 - Polarisation of the CMB (continued) - Gravitational waves and their imprints on the

Lecture 4 - Polarisation of the CMB (continued) - Gravitational waves and their imprints on the

Lecture 4 - Polarisation of the CMB (continued) - Gravitational waves and their imprints on the CMB The Single Most Important Thing You Need to Remember Polarisation is generated by the local quadrupole temperature anisotropy , which is

705 views • 55 slides
Reionization: When How - What is left ? CMB : T and polarisation large and small scales

Reionization: When How - What is left ? CMB : T and polarisation large and small scales

Reionization: When How - What is left ? CMB : T and polarisation large and small scales Transmission of flux in high-z objects (z=6 qsos and GRBs) Direct HeII observations (lower z than HI) Sources of ionization The IGM: Temperature

323 views • 8 slides
CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu,

CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu,

CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu, Max-Planck-Institut fr Astrophysik Higgs Centre Colloquium, Univ. of Edinburgh February 27, 2015 March 17, 2014 BICEP2s announcement January 30, 2015

805 views • 77 slides
Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of

Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of

Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of the CMB Planck Collaboration (2016) Lets understand the peak heights Silk+Landau Damping Sachs-Wolfe Sound Wave Matching Solutions We

1.19k views • 83 slides
Measurement of the double polarisation observable G with the Crystal Barrel Experiment @ ELSA

Measurement of the double polarisation observable G with the Crystal Barrel Experiment @ ELSA

Measurement of the double polarisation observable G with the Crystal Barrel Experiment @ ELSA Marcus Grner for the CBELSA/TAPS Collaboration Supported by SFB/TR 16 Helmholtz-Institut fr Strahlen- und Kernphysik der Uni Bonn Content

454 views • 23 slides
Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of

Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of

Lecture 3 - Cosmological parameter dependence of the temperature power spectrum - Polarisation of the CMB - Gravitational waves and their imprints on the CMB Planck Collaboration (2016) Silk+Fuziness Damping Sachs-Wolfe Sound Wave Planck

1.65k views • 137 slides
CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu,

CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu,

CMB Polarisation: Toward an Observational Proof of Cosmic Inflation Eiichiro Komatsu, Max-Planck-Institut fr Astrophysik Colloquium, ICTP, October 22, 2014 March 17, 2014 BICEP2s announcement Signature of Cosmic Inflation in the Sky [?]

1.03k views • 76 slides
? Polarisation monitoring Sabine Riemann, Andreas Schlicke, Andriy Ushakov (DESY) Positron

? Polarisation monitoring Sabine Riemann, Andreas Schlicke, Andriy Ushakov (DESY) Positron

? Polarisation monitoring Sabine Riemann, Andreas Schlicke, Andriy Ushakov (DESY) Positron Source Group Meeting, 28-30 October , 2009 University of Durham Outline Polarization measurement /monitoring near the sources : FAQ in discussions

266 views • 15 slides
Spin tunnel and Spin Polarisation Laurent Ranno Laboratoire Louis Nel, Grenoble Spin Tunnel

Spin tunnel and Spin Polarisation Laurent Ranno Laboratoire Louis Nel, Grenoble Spin Tunnel

Ecole Franco-Roumaine Magntisme des systmes nanoscopiques et structures hybrides Brasov, septembre 2003 Spin tunnel and Spin Polarisation Laurent Ranno Laboratoire Louis Nel, Grenoble Spin Tunnel Course Brasov sept. 2003 Laurent Ranno

1.18k views • 87 slides
On the nightglow polarisation: a new window for space weather observations? Electrons entry in

On the nightglow polarisation: a new window for space weather observations? Electrons entry in

ESWW16 18/11/2019 Lo Bosse 1 , Jean Lilensten 1,5 , Nicolas Gillet 3 , Sylvain Rochat 1 , Alain Delboulb 1 , Stephane Curaba 1 , Alain Roux 1 , Yves Magnard 1 , Magnar G. Johnsen 4 , Unni-Pia Lvhaug 6 , Pierre-Olivier Amblard 2 , Nicolas le

122 views • 10 slides
Towards fundamental physics from the cosmic microwave background Hiranya V. Peiris UCL and

Towards fundamental physics from the cosmic microwave background Hiranya V. Peiris UCL and

Towards fundamental physics from the cosmic microwave background Hiranya V. Peiris UCL and Stockholm (Part of) the Planck team C REDIT : BICEP / K ECK C OLLABORATIONS Temperature quadrupole at surface of last scattering creates polarisation

676 views • 53 slides
Lecture 4 - Cosmological parameter dependence of the temperature power spectrum (continued) -

Lecture 4 - Cosmological parameter dependence of the temperature power spectrum (continued) -

Lecture 4 - Cosmological parameter dependence of the temperature power spectrum (continued) - Polarisation Planck Collaboration (2016) Lets understand the peak heights Silk+Landau Damping Sachs-Wolfe Sound Wave ` 302 qr s /

681 views • 67 slides
Outline The goal The acceleration techniques Linear, why ? Energy and luminosity challenges

Outline The goal The acceleration techniques Linear, why ? Energy and luminosity challenges

1 Accelerators creating the initial state you dream of, the collider system Outline The goal The acceleration techniques Linear, why ? Energy and luminosity challenges nasty consequences end of lecture 1 Collider elements Polarisation e

1.41k views • 103 slides
Professionalising Markets Retailing in the 21 st century Presented by Ken Greig: Director,

Professionalising Markets Retailing in the 21 st century Presented by Ken Greig: Director,

Professionalising Markets Retailing in the 21 st century Presented by Ken Greig: Director, Greig and Stephenson Architects Home shopping and the internet Polarisation of shopping centres the death of our high streets The

501 views • 35 slides
Scalar field Hadamard renormalisation in AdS n Carl Kent University of Sheffield (Supervisor:

Scalar field Hadamard renormalisation in AdS n Carl Kent University of Sheffield (Supervisor:

Scalar field Hadamard renormalisation in AdS n Carl Kent University of Sheffield (Supervisor: Elizabeth Winstanley) Outline 1. Scalar field theory in AdS n 2. Overview of research 3. Calculation of the vacuum polarisation 2 ren

369 views • 15 slides
JRJC 2009 CEA-Saclay/IRFU/SPhN et la Fondation Nationale de Science. SPIN INTRINS QUE Le spin

JRJC 2009 CEA-Saclay/IRFU/SPhN et la Fondation Nationale de Science. SPIN INTRINS QUE Le spin

tudes sur Le Rle de la Polarisation des Gluons dans le Spin Total du Proton Par la Production de Hadrons Astrid Morreale JRJC 2009 CEA-Saclay/IRFU/SPhN et la Fondation Nationale de Science. SPIN INTRINS QUE Le spin est une proprit

570 views • 42 slides

More recommend