2017-03 – Finite Size Scaling in 2D Causal Set Quantum Gravity
DIAS-STP-17-03
Finite Size Scaling in 2D Casual Set Quantum Gravity
L. Glaser, D. O’Connor and S. Surya
This preprint is available on Arxiv.org
This preprint is available for download :
Details provided:
- Date of publication : 20/06/17
To obtain copies of any of the preprints in the archives, please contact us and specify the preprint number(s), author(s), title(s) and number of copies wanted.
2017-02 – Rational CFTs on Riemann surfaces
DIAS-STP-17-02
Rational CFTs on Riemann surfaces
M. Leitner and W. Nahm
This preprint is available on Arxiv.org
This preprint is available for download :
Details provided:
- Date of publication : 22/05/17
To obtain copies of any of the preprints in the archives, please contact us and specify the preprint number(s), author(s), title(s) and number of copies wanted.
2017-01 – An algebraic approach to minimal models in CFTs
DIAS-STP-17-01
An alegbraic approach to minimal models in CFTs
M. Leitner
This preprint is available on Arxiv.org
This preprint is available for download :
Details provided:
- Date of publication : 22/05/17
To obtain copies of any of the preprints in the archives, please contact us and specify the preprint number(s), author(s), title(s) and number of copies wanted.
Mon 26th June – Team of Astronomers led by DIAS Astronomer Use Alma to Make the Most Detailed Image of Another Star that has Ever Been Produced
An international team of astronomers have used ALMA (Atacama Large Millimeter/submillimeter Array), the world’s largest radio telescope, to make the most detailed image of the surface of a star (other than our Sun) that has ever been created at radio wavelengths. The image was taken of Betelgeuse, the famous Red Supergiant located in the constellation Orion, and remarkably reveals that the temperature in its inner atmosphere is far from uniform. The discovery could help explain how the atmospheres of these stars are heated and how material from these stars is transported to the interstellar medium.
“ALMA now provides us with the capabilities to image surface features on nearby stars while also directly measuring the temperature of these features” explains Dr. Eamon O’Gorman, an Irish Research Council Fellow and Astronomer at the Dublin Institute for Advanced Studies, who led the team. “We have known for decades that the visible surface of Betelgeuse is not uniform, but ALMA has now shown in beautiful detail that the temperature in its inner atmosphere is also not uniform. It looks like these temperature fluctuations could be caused by magnetic fields, similar to what we see on the Sun, our nearest star.” The team’s results have recently been published in the journal ‘Astronomy & Astrophysics’.
In terms of size, Betelgeuse is enormous, being about 1400 times larger than our Sun, and more than one billion times larger in terms of volume. As stars like Betelgeuse evolve, they expel an enormous amount of themselves back into the interstellar medium via stellar winds. These winds contain crucial heavy elements that the stars have manufactured and are vital ingredients for the next generation of stars and planets.
“Located about 650 light years away, Betelgeuse is certainly not the closest star to our solar system, but its sheer size makes it an ideal target to image directly with ALMA”, says Dr. Pierre Kervella, astronomer at the Paris Observatory and member of the team, he continued, “When we look at the night sky with our naked eyes, we see bright stars everywhere, but because they are so small, even the most powerful telescopes in the world struggle to image their surfaces. Our results show ALMA has the capability to image the surfaces of the largest stars in detail.”
Consisting of 66 gigantic 12-metre and 7-metre antennas, ALMA is the most powerful radio telescope in the word. The telescopes can separate over distances of 16 kilometres, giving ALMA an extraordinarily powerful “zoom”. ALMA is an international astronomy facility located at 5000 metres altitude at Chajnantor in northern Chile, at one of the driest sites in the world. ALMA is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile and is the world’s largest astronomy project.
Image 1:
The new ALMA image of Betelgeuse. The overplotted circles allow the size of Betelgeuse to be compared to the size of the orbits of the planets in our solar system.
(Credit: ESO/ALMA/P. Kervella)
Image 2:
ALMA on the Chajnantor Plateau, located at an altitude of 5000 meters in the Chilean Andes. ALMA consists of 66 individual antennas which combine their signals together and can be separated by distances of up 16 kilometres.
Credit: Clem & Adri Bacri-Normier (wingsforscience.com)/ESO
Dr Colm Bracken

Name: Dr Colm Bracken
Title: Post Doctoral Research Fellow
E-Mail: cbracken@cp.dias.ie
Phone: +353 1 4406656 ext 352
Address: 31 Fitzwilliam Place, Dublin 2 D02-XF86
Research Interests: Optical/near-IR MKID detectors and read-outs, Far-IR TES detectors and feed systems, Numerical modelling for EM/RF/microwave simulation, and Quasi-optical analysis and design.
Biographical Sketch :
Colm studied physics with astrophysics at National University of Ireland, Maynooth, graduating in 2010. He received his PhD in 2015 from N.U.I. Maynooth for his research in electromagnetic analysis and design of far-infrared receivers and detectors for the SAFARI instrument on the SPICA space telescope, as part of a collaboration between ESA, N.U.I. Maynooth, SRON (the Netherlands), among other instututes. From 2015 to 2016 he worked as a postdoctoral researcher on the EU-FP7 funded FISICA (Far-Infrared Space Interferometer Critical Assessment) project, designing a baseline quasi-optical layout for a proposed double-Fourier interferometer space mission.
Colm held a temporary Lecturer/Asst. Professor position at University College Dublin from 2016 to 2017, lecturing undergraduate and graduate modules including Galaxies, Cosmology and the ISM; Space Mission Design; Gamma-ray Space Detectors Advanced Lab; Cubesat Subsystems Advanced Lab; while continuing his research in far-infrared instrumentation and simulation. He is now a postdoctoral researcher at the Dublin Institute of Advanced Studies, working with Professor Tom Ray on large-format arrays of Microwave Kinetic Inductance Detectors for optical/near-infrared wavelengths.
Selected Publications:
1) Quasi-optical analysis of a far-infrared spatio-spectral space interferometer concept http://adsabs.harvard.edu/abs/2016InPhT..77..171B
2) MUSE – Mission to the Uranian system: Unveiling the evolution and formation of ice giants http://adsabs.harvard.edu/abs/2015AdSpR..55.2190B
3) Progress in spectral-spatial interferometry at multi-THz frequencies — Potential applications http://ieeexplore.ieee.org/abstract/document/7460625
4) Optical modeling of waveguide coupled TES detectors towards the SAFARI instrument for
SPICA http://adsabs.harvard.edu/abs/2012SPIE.8452E..0LT
Dr Alessio Carrati o Garatti
Alessio Caratti o Garatti Dr., former Post Doctoral Research Fellow 2014-2017
Thursday 6th July: STP Seminar – “Quantum engineering using magnetic fields: Quantum Magnetomechanics”
Title: Quantum engineering using magnetic fields: Quantum Magnetomechanics
Speaker: Jason Twamley (Macquarie University, Sydney)
Abstract: Optomechanics – the control and manipulation of mesocopic objects towards the quantum regime, has attracted much attention. The use of light however, brings with it several problems, scattering noise being just one. In this talk we introduce a new approach to control the quantum motion of mescoscopic objects using magnetic fields. We describe our proposal to levitate and cool superconducting objects using magnetic fields and superconducting quantum circuits, how such levitated objects can be used for high precision gravimetry, specific experimental designs for ultra-strong and deep strong coupling using magnetomechanics and how one can engineer spin squeezing and spin Cats using magnetomechanics.
Time: Thursday 6th July 2017, 2.30pm.
Place: Seminar Room, School of Celtic Studies, DIAS, 10 Burlington Road, Dublin 4.
Graham Kells Paper: Physical Review B – Editor’s Suggestion
‘Parafermionic clock models and quantum resonance’:
A paper co-authored by Dr Graham Kells (STP) has been noted as ‘Editor’s Suggestion’ in the current issue of Physical Review B.
16 – 18 June 2017 : Solarfest 2017 at Dunsink Observatory

Solarfest will take place at Dunsink Observatory, Castleknock, Dublin 15 on the 16th, 17th and 18th of June. Organised by the Dublin Institute for Advanced Studies (DIAS), Irish Federation of Astronomical Societies (IFAS), Meath Astronomy Group and the TCD Solar Group, this annual event is a celebration of solar astronomy for professional and amateur astronomers, as well as the general public.
The free event consists of a public open evening on Friday 16th June, an all-day public event on Saturday 17th June and an afternoon family event on Sunday 18th June. The events include talks by enthusiastic astronomers, access to/tours of the observatory, and solar observing if the weather permits.
Solarfest is a fun way to find out more about the Sun and its place among the other stars, as well as its crucial importance to Earth. Dr. Jonathan Mackey, an astrophysics research fellow in DIAS and one of the main organisers of Solarfest, comments: “The Sun is our nearest star, and our understanding of all other stars is based on how much we know about the Sun. Observations and models of the Sun and its wind are important for developing theoretical models of the atmosphere and surface conditions on planets that are being discovered around other stars.”
Michael O’Connell, amateur astronomer from IFAS says, “Solarfest provides an excellent opportunity for Ireland’s finest scientists to come together with amateur astronomers and the general public to share their latest research in solar astronomy in the relaxed setting of Dunsink Observatory. Events such as Solarfest play a crucial role in promoting Science, Technology, Engineering & Maths (STEM) and ensuring the next generation can explore and discover fulfilling careers here in Ireland.”
Find out more, and book free tickets at https://www.dunsink.dias.ie/solarfest/
For further information contact:
- Jonathan Mackey at 087 176 0756 or by email at jmackey@cp.dias.ie
- Hilary O’Donnell/Sullivan at 087 629 4966 (Official Dunsink Obs. phone number, available at any time) or by email at hod@cp.dias.ie
15th Dec #DIASDublin talk The Physics & Astrophysics of Merging Neutron-Star Binaries by Luciano Rezzolla @goetheuni bit.ly/2xiMz3y
#DIASDublin Annual Report 2016 published today. The press release is available here - bit.ly/2hceXi5
17th November @ 8pm – #DIASDublin School of Celtic Studies Statutory Public Lecture 2017 taking place @tcddublin
DIAS Giovanna Tinetti Lecture "Brave new worlds: the planets in our galaxy" youtu.be/le0Kh0JxMMA via @YouTube

















