Content The Pierre Auger Observatory Particle detectors at home The VATLY Radio telescope

1. Research at VATLYP.N. Diepfor P.T. Anh, P. Darriulat, P.N. Dong, D.T. Hoai, P.T. Nhung, N.T. Phuong and N.T. Thao(Institute for Nuclear Science and Technolgy, Hanoi, Vietnam)Quy Nhon, August, 2013

2. Content • The Pierre Auger Observatory • Particle detectors at home • The VATLY Radio telescope • Radio astronomy • Teaching and training • Conclusion

3. THE PIERRE AUGEROBSERVATORY

4. VATLY and PAO Vietnam Auger Training LaboratorY was created twelve years ago (with material and instruments given to us as gifts from CERN research teams of all over the world) in association with the Pierre Auger Observatory (PAO). The PAO covers 50×60 km2 in Argentina and studies the ultra high energy cosmic rays (UHECRs, 1018 to 20 eV). UHECRs are extragalactic; their sources and nature are unknown. The PAO includes 1700 Cherenkov ground detectors, 1.5 km apart from each other, and 24 UV telescopes measuring the shower fluorescence in the atmosphere.

5. Mass composition: at higher energies, “all sky” move from protons to Fe, but insufficient statistics for Cen A and AGN’s to be confirmed. The PAO has obtained evidence for the GZK cut-off (photoproduction on the CMB) and for a positive but weak correlation with nearby galaxies (Centaurus A).

6. VATLY contributions include: A study of low amplitude signals and the detection of decay electrons from stopping muons; A measurement of shower divergences; Contributions to the identification of the primaries (protons or iron) from the muon density on ground; Identification of primaries from Cen A; Response of the PAO PMTs as a function of photon impact (in Hanoi). Detailed studies of long term stability and ageing of the PAO detectors;Shower development studies. The next generation of cosmic ray observatories will take at least one decade to mature. In the past two to three years, the interest of the team has been progressively shifting away from cosmic ray studies to radio astronomy where the time scale and size of the research projects are better adapted to a small, young and isolated group such as ours. Without the Pierre Auger Collaboration, we would not have been able to take off and come of age: our gratitude for their constant and friendly support is immense.

7. In our conversion from cosmic ray physics to astrophysics and radio astronomy, we enjoy moral and material support from astrophysicists, in particular in France and at IAU, whom we express here our deepest gratitude. The choice of radio astronomy as a particular branch of astrophysics was dictated by a combination of physics motivations (its presence at the forefront of most current explorations on the frontier of modern astrophysics) as well as by arguments of convenience (influence and encouragements of Pr NQ Rieu, presence in Viet Nam of Drs DV Trung and PB Ngoc, near impossibility to make observations in the visible under the foggy tropical sky).

8. PARTICLEDETECTORSAT HOME

9. Early studies explored some features of the cosmic ray flux in Hanoi where the rigidity cut-off reaches its world maximum of 17 GV. In particular, we measured the muon flux, its zenith angle dependence and the east-west asymmetry.

10. #4 #3 80 120 162 #5 #6 Cable hole We assembled a replica of a PAO ground detector on the roof of the laboratory and added three smaller counters allowing for an unbiased shower trigger. It is used for training and for making detailed studies of its response.

11. THE VATLY RADIO TELESCOPE

12. Three years ago, we acquired a 2.6 m diameter radio telescope tuned on (and around) the 21 cm hydrogen line. It has been used to map HI in the disk of the Milky Way and is currently taking data on the Sun at its maximum of activity.Accurate frequency spectra are collected every 8 seconds displaying very clearly the 21 cm line.

13. Velocity Doppler spectra have been collected along the disk of the Milky Way over three quarters of the galactic longitude. They show evidence for differential rotation.Each spectrum has been reduced into peaks associated with different clouds of atomic hydrogen. Doppler velocity wrt Sun Galactic longitude

14. A map of atomic hydrogen in the Milky Way disk has been constructed and compared with the known arm and bar structure. Spitzer Ambiguous Unambiguous Peak positions Map of power density

15. The Sun, which is this year at its maximum of activity, has been tracked for several months. A joint analysis of the collected data with similar data taken by the Learmonth Solar Observatory in Australia has shown the presence of flares and has given evidence for mHz oscillations at the percent level (published in Solar Physics); additional observations are necessary to understand their origin (see P.T. Nhung’s presentation at the Conference). Hanoi Learmonth

16. HA NOI LEARMONTH The peculiar position of Ha Noi on the geomagnetic equator, which is causing the high rigidity cut-off for cosmic ray detection, is also causing an exceptionally high scintillation index (meaning strong inhomogeneities in the ionosphere) which might be a source of multipathing (interferences between different photon paths).

17. RADIO ASTRONOMY

18. In the context of two PhD theses made under joint supervision with astrophysicists abroad (where the students spend 4 months a year during three years), we collaborate with French institutes on the study of data collected on large installations, in particular the Plateau de Bure radio interferometer (PdBI).

19. G’ A3 HST B A2 G A1 Under supervision of Dr Frederic Boone (IRAP, Toulouse) Tuan Anh studies the host galaxy of a gravitationally lensed high redshift quasar (z~2.8, look back 11.3 Gyr), RXJ0911. Detection of the CO(7-6) line measures its gas content and the continuum below its dust content, providing useful information on the star formation rate in such early galaxies.

20. Lensing is complicated by the fact that the extended source overlaps the lens caustic. We studied this peculiar situation in detail (published in Research in Astronomy and Astrophysics) ~3”

21. The results show that the source has a radius of 850±120 pc on the line (~7 s.d.) and 260±130 pc (only 2 s.d.) in the continuum. They also provide evidence for ellipticity and for a significant velocity gradient (molecular outflow and/or rotation)(Preliminary results published in Astronomy and Astrophysics Letters) No velocity gradient Ellipticity: 3.3 s.d. away from circular Evidence for velocity gradient at 4.5 s.d. Pot. 2 Pot. 1 arcsec

22. Under supervision of Dr Thibaut Le Bertre (LERMA, Paris) Hoai studies an Asymptotic Giant Branch star in its thermal pulsing phase, RS Cnc, using high resolution PdBI data on the CO(1-0) and CO(2-1) lines and VLA data on HI. The star features a bipolar molecular outflow with a wind velocity of ~8 km/s, superimposed on a lower velocity wind (~2 km/s). Detailed studies of the velocity spectra allow for constructing a model of the star atmosphere accounting for many, but not all, of the observed features.

23. 1.4 mas 20 km/s 1.4 mas

24. TEACHING ANDTRAINING

25. From the beginning we have given high priority to the promotion of astrophysics in Vietnam, from where it is essentially absent, by giving university lectures at the Hanoi University of Sciences (Intron to astrophysics and cosmology); lectures at Summer Schools in Hanoi (Intron to cosmology, IAU), in Da Nang (Black holes, recent advances, VSOP/CNRS), in Saigon and Quy Nhon (Intron to cosmic rays, IAU); Public lectures in Hanoi (Ha Noi à l’écoute du cosmos) and in Saigon (Astrophysics and Vietnam). We now contribute lab work (SRT, particle detectors, radiowaves) to the University of Science and Technology of Hanoi master Space & Applications (Alain Maestrini, Yannick Giraud-Heraud et al). In May this year, we invited to Ha Noi F. Combes, T. Le Bertre and F. Boone to give lectures on topics related to the PhD research work of Tuan Anh and Hoai.

26. We do our utmost to establish close contacts with astronomers and astrophysicists in the region and abroad.In particular with the two astrophysicists doing active research in Vietnam (Pr Dinh Van Trung in Ha Noi and Pr Phan Bao Ngoc in Saigon) and with Pr Nguyen Quynh Lan who is heading the Department of Astronomy at the Ha Noi University of Education. Several VATLY members have attended Summer schools on astrophysics in Ha Noi, Saigon, Grenoble and Granada (Tuan Anh and Hoai, IRAM), in Castelgandolfo (Hiep, Pontifical Academy), in Li Jiang (Tuan Anh, IAU) and/or astrophysics/cosmology conferences in the region (the whole team in Vinh, Nhung and Diep in Quy Nhon, Thao in Malaysia, Hiep and Nhung in Philippines, Tuan Anh in Thailand, Nhung and Diep in China).We joined SEAAN, the South East Asia Astronomy Network and SEAYAC, the South East Asian Young Astronomers Collaboration and have strongly contributed to the creation of a Vietnam Astrophysics Group collecting the few of us who, in Vietnam, are acting for the promotion of training and research in modern astrophysics.

27. Undergraduate dissertations Study of the effect of atmospheric pressure on the cosmic muon rate in Ha Noi Study of the effect of temperature on the cosmic muon rate in Ha Noi Measurement of the muon life time A simple model of the longitudinal development of electromagnetic showers The black hole in the centre of the Milky Way Optical properties of a Cherenkov counter Huong 2008 Galaxy collisions as possible sources of ultra high energy cosmic rays Extensive air showers and LPM effect X ray binaries and three body capture Global warming and cosmic rays Gravitational lensing and Einstein rings Construction, operation and exploitation of a scintillator hodoscope Diep 2003 Lion 2009 Nhung 2003 Hoai 2009 Huyen 2005 Hiep 2010 V.Phuong 2006 Dung 2011 K.Phuong 2006 Phuong 2013 The 2007

28. Master theses Measurement of the east-west asymmetry of the cosmic muon flux in Ha Noi Performance study of water Cherenkov counters The Cherenkov counters of the VATLY laboratory Detection and study of ultra-high energy cosmic rays An original approach to the simulation of the development of extensive air showers up to extreme high energies Duong 2003 Thao 2007 The detection of extensive air showers in Ha Noi Radio detection of the Sun Diffusive shock acceleration in SNR shocks Observation of the 21cm sky using the VATLY radio telescope Nhung 2006 T. Anh 2010 Dong 2006 The 2010 Diep 2006 Hiep2012 Hoai 2012

29. PhD Theses (+Tuan Anh and Hoai in the mill) Measurement of the angular distribution of the cosmic muon flux in Ha Noi Contribution to the study of extensive air showers using the surface detector of the Pierre Auger Observatory Contribution to the study of the response to Cherenkov photons of a large diameter photomultiplier tube and of its use at the Pierre Auger Observatory Contribution to the identification of the nature of ultra high energy cosmic rays at the Pierre Auger Observatory The VATLY Cherenkov detector and its response to electrons and muons Thieu 2006 Nhung 2009 Dong 2010 Diep 2010 Thao 2013

30. CONCLUSION

31. Particle physics and astrophysics are not significantly supported in Vietnam and only a very few individuals do research in these fields, in the wake of contacts they had with research teams abroad, where they studied for their PhD. Experimental physics is still too often belittled with respect to theoretical physics. Progress implies making the science top deciders aware of the importance of encouraging and supporting teams as much as individuals, of making room for fundamental research at the frontier of knowledge, of spelling out a clear scientific research policy for the country. There is still a long way to go but we hope for the future creation of a research institute that would favor the progress and development of such research.

32. In order to survive, not to mention to progress, we need to work in close collaboration with foreign colleagues.I take this opportunity to express our deepest gratitude for the help and support that they give us.We receive invaluable support from the World Laboratory in the form of fellowships. In Vietnam, we enjoy financial support from the Institute for Nuclear Science and Technology, which hosts us, and from the National Foundation for Science and Technology Development (NAFOSTED).We are also grateful to IN2P3/CNRS, the French Embassy, Rencontres du Vietnam and Odon Vallet fellowships for occasional support.

33. THANK YOU FOR YOUR ATTENTION!