ICTP - Virtual Seminars

Virtual Seminars

ICTP is expanding its free, online, interactive streaming options for its seminars and colloquia to mitigate some of the effects of isolation during the COVID-19 emergency and beyond. Check this page frequently for upcoming events that will be shared via the interactive webinar platform Zoom.

Showing 21 records

Europe/Rome The percolation properties of random fields arise naturally in many contexts, ranging from planet science to transport in disordered systems. In this talk we will discuss new results concerning the percolation transition of long-range correlated random fields. In particular we show that the level sets of surfaces with negative Hurst exponent are conformal fractals. Moreover, we revisit and solve the long-standing problem of the percolation transition in the 2D Gaussian Free Field (GFF). We show the existence of a non-trivial transition where the level set of the GFF become "logarithmic fractals". The correlation function of such fractals is also exactly computed. VIRTUAL ICTP pio@ictp.it

Seminar

26 Jan 2021

@ VIRTUAL

Condensed Matter and Statistical Physics

CMSP Seminar (Joint ICTP/SISSA Statistical Physics): The Topography of Random Surfaces: Percolation Transitions and Conformal Fractals

Speaker(s): Raoul SANTACHIARA (Univ. Paris-Sud, LPTMS, Orsay, France)

Seminar Start Time: 11:00

Europe/Rome You are cordially invited to participate in the Graduation Ceremony of the students of the 6th cycle of the Master of Advanced Studies in Medical Physics, a two-year advanced training programme in the field of medical physics, jointly organised by ICTP and the Trieste University and co-sponsored by the International Atomic Energy Agency (IAEA). The first year is spent at ICTP while the second year is dedicated to clinical professional training in a Medical Physics Department of an Italian hospital of the training network, supported by the Italian Association of Medical Physics (AIFM). The International organisation for medical physics (IOMP) has given an international accreditation to the programme. The programme is supporting LMI countries in the development of medical physics, an applied physics sector contributing to the development, introduction and use of advanced technologies in the medical sector. Including the 12 students of this 6th cycle, so far the programme has graduated 97 medical physicists (32% female) from about 60 countries (45 from Africa, 24 from Asia, 21 from Latin America and Caribbean, 6 from Europe and 1 from Oceania). Register in advance for this webinar: https://zoom.us/webinar/register/WN_V5K2EomDSK6cxcxbIFOk9w After registering, you will receive a confirmation email containing information about joining the webinar. Should you not be able to join the Webinar, the Colloquium is also available in live streaming at: ictp.it/livestream. The tentative programme outline is as follows: Introduction: Luciano Bertocchi (ICTP), followed by Atish Dabholkar (ICTP Director), Valter Sergo (Trieste University), Deborah van der Merwe (Human Health Dept, IAEA), Slavik Tabakov (IOMP Past President, IUPESM Vice-President), Michele Stasi (AIFM), Ahmed Meghzifene (MMP External Advisor), Representative of EFOMP (tbc) Brief remarks: invited guest (tbc) Invited lecture: “Pros and Cons of Particle Therapy General overview, state of the art, future perspectives” by Professor Marco Durante (GSI, Darmstadt, Germany) Degrees distribution to graduating students (Renata Longo and Atish Dabholkar). All are welcome to attend. Online ICTP pio@ictp.it

Ceremony

26 Jan 2021

@ Online

GRADUATION CEREMONY: Master of Advanced Studies in Medical Physics (2019/2020)

As of 2020, a total of 122 students have arrived at ICTP for the combination of theoretical and practical training offered by the Masters in Medical Physics programme since it was inaugurated in 2014. These new graduates will play key practical roles in healthcare as highly trained medical physicists, involved in both individual and public health.

Europe/Rome David Spergel is the director of the Center for Computational Astrophysics. His research interests range from the search for planets around nearby stars to the shape of the universe. Since completing his Ph.D. work, he has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, he has measured the age, shape and composition of the universe. His observations have played a significant role in establishing the standard model of cosmology. Spergel is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is co-chair of the Nancy Grace Roman Space Telescope (formerly known as WFIRST) science team. The Roman Telescope will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. After 30 years at Princeton, Spergel is now retired and full-time at the Simons Foundation, and Charles Young Professor of Astronomy Emeritus on the Class of 1897 Foundation at Princeton University where he was department chair for nearly a decade. He is associate faculty member in both the department of physics and the department of mechanical and aerospace engineering at Princeton. He has been the mentor of 32 graduate students, 35 postdoctoral fellows and 60 undergraduates, and continues to advise and mentor graduate students at Princeton. Spergel is a member of the National Academy of Sciences in 2007, a member of the American Academy of Arts and Sciences in 2012 and was elected a Legacy Fellow of the American Astronomical Society in 2020. His work has been recognized with the Warner Prize and the Heinemann Prize, the MacArthur Fellowship, Shaw Prize, Gruber Prize, and the Breakthrough Prize in Fundamental Physics. Abstract for the Colloquium: Observations of the cosmic microwave background and measurements of the large-scale structure of the universe have revealed the initial fluctuations that grew to form galaxies. I will review measurements showing that these fluctuations were Gaussian random phase and that the basic properties of the universe appear to be described by the Lambda Cold Dark Matter model. I will report recent results from the Atacama Cosmology Telescope that probe not only the initial conditions but also map the integrated matter density, integrated pressure and integrated electron monentum through gravitational lensing and the Sunyaev-Zel’dovich Effects. Register in advance for this webinar: https://zoom.us/webinar/register/WN_3YbVuQHIQ4m4MZYw7svSqQ After registering, you will receive a confirmation email containing information about joining the webinar. Should you not be able to join the Webinar, the Colloquium is also available in live streaming at: ictp.it/livestream The Lecture Series takes place on 27, 28 and 29 January 2021 at 16.00 hrs each day on the same Zoom ID. The Abdus Salam Distinguished Lecture Series receives generous support from the Kuwait Foundation for the Advancement of Sciences (KFAS). For more information see: https://kfas.ictp.it/ ICTP pio@ictp.it

Seminar

27 Jan 2021

Salam Distinguished Lectures 2021 by Prof. David Spergel. Lecture 1: "What the Universe’s Baby Picture Reveals About Fundamental Physics"

Room: Online

Speaker(s): Prof. David Spergel, Center for Computational Astrophysics, Flatiron Institute, USA

Seminar Start Time: 16:00

Europe/Rome David Spergel is the director of the Center for Computational Astrophysics. His research interests range from the search for planets around nearby stars to the shape of the universe. Since completing his Ph.D. work, he has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, he has measured the age, shape and composition of the universe. His observations have played a significant role in establishing the standard model of cosmology. Spergel is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is co-chair of the Nancy Grace Roman Space Telescope (formerly known as WFIRST) science team. The Roman Telescope will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. After 30 years at Princeton, Spergel is now retired and full-time at the Simons Foundation, and Charles Young Professor of Astronomy Emeritus on the Class of 1897 Foundation at Princeton University where he was department chair for nearly a decade. He is associate faculty member in both the department of physics and the department of mechanical and aerospace engineering at Princeton. He has been the mentor of 32 graduate students, 35 postdoctoral fellows and 60 undergraduates, and continues to advise and mentor graduate students at Princeton. Spergel is a member of the National Academy of Sciences in 2007, a member of the American Academy of Arts and Sciences in 2012 and was elected a Legacy Fellow of the American Astronomical Society in 2020. His work has been recognized with the Warner Prize and the Heinemann Prize, the MacArthur Fellowship, Shaw Prize, Gruber Prize, and the Breakthrough Prize in Fundamental Physics. Abstract for the public talk: Observations of the microwave background, the left-over heat from the big bang, the large-scale distribution of galaxies and the properties of distant supernova have led to a remarkable simple model for our universe. With only five parameters (the density of atoms, the density of matter, the age of the universe, the amplitude of fluctuations in the early universe and their scale dependance), this model can fit a host of astronomical observations. We have now determined these basic parameters at the few percent level or better. While simple, our universe is very strange. Atoms make up only 5% of the universe, most of the universe is made of mysterious dark matter and dark energy. We do not understand how the universe began or why there is more matter than anti-matter. I will review our current understanding and look forward to future measurements that can address these big open questions. Register in advance for this webinar: https://zoom.us/webinar/register/WN_3YbVuQHIQ4m4MZYw7svSqQ After registering, you will receive a confirmation email containing information about joining the webinar. Should you not be able to join the Webinar, the Colloquium is also available in live streaming at: ictp.it/livestream The Lecture Series takes place on 27, 28 and 29 January 2021 at 16.00 hrs each day on the same Zoom ID. The Abdus Salam Distinguished Lecture Series receives generous support from the Kuwait Foundation for the Advancement of Sciences (KFAS). For more information see: https://kfas.ictp.it/ ICTP pio@ictp.it

Seminar

28 Jan 2021

Salam Distinguished Lectures 2021 by Prof. David Spergel: Lecture 2: “Our Simple Strange Universe”

Room: Online

Speaker(s): Prof. David Spergel, Center for Computational Astrophysics, Flatiron Institute, USA

Seminar Start Time: 16:00

Europe/Rome The 2019 Dirac Medal and Prize Ceremony which was due to take place in May 2020 during the ICTP Summer School on Cosmology 2020 has been re-scheduled to Friday 29 January 2021 starting at 13.30 hrs and will be online. ICTP awarded its 2019 Dirac Medal and Prize to three physicists whose research has made a profound impact on modern cosmology. Viatcheslav Mukhanov (Ludwig Maximilian University of Munich), Alexei Starobinsky (Landau Institute for Theoretical Physics) and Rashid Sunyaev (Max Planck Institute for Astrophysics) share the prize for “their outstanding contributions to the physics of the Cosmic Microwave Background (CMB) with experimentally tested implications that have helped to transform cosmology into a precision scientific discipline by combining microscopic physics with the large scale structure of the Universe.” All three winners have made important contributions to the understanding of the early Universe in the context of inflationary cosmology. Dirac Medal lectures (25 mins each) are as follows: * "How predictive are cosmological theories?" by Professor Viatcheslav Mukhanov. Abstract: I will discuss the robust model independent predictions of the theory of quantum origin of the universe structure and confront them with the results of the recent measurements of the CMB fluctuations. * "Beginning the Universe from the maximally symmetric state in the past" by Professor Alexei A. Starobinsky. Abstract: The radical hypothesis that our Universe was in the maximally symmetric state during some period in its remote past, as much symmetric with respect to both quasi-classical background and small quantum perturbations upon it as physical laws permit this, has been realized in some rather narrow class of slow-roll inflationary models and has led to quantitative predictions about the power spectra of primordial scalar and tensor inhomogeneous perturbations which have been confirmed by observations in the former case. From the theoretical point of view, these models provided us with the wonderful possibility to apply the previously developed quantum field theory in curved space-time, more concretely, the quantum-gravitational effect of creation of particles and field fluctuations in cosmological backgrounds, to phenomena observable at the present time. The simplest viable inflationary models which I shall discuss have only one adjustable dimensionless parameter to be taken from observations. They correctly predicted deviation of the primordial scalar spectrum from the exactly scale-invariant one (n_s =1), where n_s is the spectral slope, by relating this small quantity to the ratio of the Hubble constant to the present CMB temperature. Their next most important target prediction is about the purely quantum-gravitational effect: the amplitude of primordial tensor perturbations (gravitational waves) in terms of the relation between the tensor-to-scalar ratio r and n_s: r = 3(1- n_s)^2. However, nature may require more parameters for the phenomenological description of the inflationary stage, in particular, if some of already discovered black holes would be proven to be primordial. * "The X-Ray map of the Universe with a million accreting supermassive black holes and tens of thousands of clusters of galaxies" by Professor Rashid Sunyaev. Abstract: The Orbital Observatory “Spektr-RG” (SRG) was launched to the halo orbit around the L2 point 1.5 million km away from the Earth with the PROTON launcher on July 13th, 2019. It scanned the whole sky twice already and created the map of the Universe and the “Milky Way” Galaxy in X-Rays. More than a million supermassive accreting black holes in quasars and Active Galactic Nuclei at cosmological distances up to z=6.2 are detected already. The observations of the clusters of galaxies (most massive gravitationally bound objects in the Universe) demonstrated that X-Ray sky surveys could still compete with the microwave SZ-effect sky surveys. We plan to use this giant amount of bright objects at high z to study the growth of the large scale structure of the Universe using Baryonic Acoustic Oscillations and other cosmological tests during and after reionization. I plan to mention the discovery of “eRosita Bubbles” above and below the plane of our Galaxy, detection of X-Ray emission from hundreds of stars with exoplanets, Tidal Disruption Events and very strong variability of the X-Ray sky on the half a year time scale. REGISTER FOR THE EVENT: Register in advance for this webinar: https://zoom.us/webinar/register/WN_mavq6fWGSlWo_ueIj-amsg After registering, you will receive a confirmation email containing information about joining the webinar. Should you not be able to join the Webinar, the Colloquium is also available in live streaming at: ictp.it/livestream. A detailed programme outline will be available shortly. About the ICTP Dirac Medal First awarded in 1985, ICTP's Dirac Medal is given in honor of P.A.M. Dirac, one of the greatest physicists of the 20th century and a staunch friend of the Centre. It is awarded every year on Dirac's birthday, 8 August, to scientists who have made significant contributions to theoretical physics. For more details about the prize and a list of past winners, see: https://www.ictp.it/about-ictp/prizes-awards/the-dirac-medal.aspx. ICTP pio@ictp.it

Ceremony

29 Jan 2021

2019 Dirac Medal and Prize Ceremony

Room: Online

2019 Dirac Medal lectures: "How predictive are cosmological theories?" (Professor Viatcheslav Mukhanov) "Beginning the Universe from the maximally symmetric state in the past" (Professor Alexei A. Starobinsky) "The X-Ray map of the Universe with a million accreting supermassive black holes and tens of thousands of clusters of galaxies" (Professor Rashid Sunyaev) The Dirac Medal and Awards Ceremony will be followed by the third talk in the 2020 Salam Distinguished Lecture Series (on a separate Zoom platform - see below).

Europe/Rome Register in advance for this meeting: https://zoom.us/meeting/register/tJ0ucuypqjorG9DEWT_unX9mtbmwHXtsw5b7 After registering, you will receive a confirmation email containing information about joining the meeting. Abstract: In this talk I will discuss the notions of an optimal symplectic connection and stability of fibrations. The former is a PDE for a canonical choice of fibrewise constant scalar curvature Kähler (cscK) metric, for a fibration whose fibres admit cscK metrics. The latter is a notion of algebro-geometric stability for such fibrations. The goal of the talk is to explain what these notions are, partly in preparation for Michael Hallam's talk the following week. I aim to explain how the notions arose, and how they specialise to the Hermite-Einstein equation and slope stability, respectively, for the underlying vector bundle, when the fibration is the projectivisation of a vector bundle. I will survey some of the results known about these notions, and how they are related. This is joint work with Ruadhaí Dervan. Zoom event ICTP pio@ictp.it

Seminar

29 Jan 2021

@ Zoom event

Mathematics

ICTP/SISSA Math Seminar on Kähler Geometry: Optimal symplectic connections and stability of fibrations

Speaker(s): Lars Sektnan (Aarhus University)

Seminar Start Time: 14:00

Europe/Rome David Spergel is the director of the Center for Computational Astrophysics. His research interests range from the search for planets around nearby stars to the shape of the universe. Since completing his Ph.D. work, he has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, he has measured the age, shape and composition of the universe. His observations have played a significant role in establishing the standard model of cosmology. Spergel is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is co-chair of the Nancy Grace Roman Space Telescope (formerly known as WFIRST) science team. The Roman Telescope will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. After 30 years at Princeton, Spergel is now retired and full-time at the Simons Foundation, and Charles Young Professor of Astronomy Emeritus on the Class of 1897 Foundation at Princeton University where he was department chair for nearly a decade. He is associate faculty member in both the department of physics and the department of mechanical and aerospace engineering at Princeton. He has been the mentor of 32 graduate students, 35 postdoctoral fellows and 60 undergraduates, and continues to advise and mentor graduate students at Princeton. Spergel is a member of the National Academy of Sciences in 2007, a member of the American Academy of Arts and Sciences in 2012 and was elected a Legacy Fellow of the American Astronomical Society in 2020. His work has been recognized with the Warner Prize and the Heinemann Prize, the MacArthur Fellowship, Shaw Prize, Gruber Prize, and the Breakthrough Prize in Fundamental Physics. Abstract for the seminar talk: Can we go beyond measuring the power spectrum of the cosmic microwave background and recover the universe’s initial conditions? I will begin by describing some of teh observational programs that will give us a more complete picture of the large-scale structure of the universe: the Rubin Observatory, the Euclid Telescope, DESI, the Roman Space Telescope and the Simons Observatory. I will then ask whether we can forward model the universe from initial conditions to match these data sets. This challenging problem will require the use of machine learning techniques to enable rapid forward modeling of the universe. I will describe recent efforts by our group at Flatiron in this area. Register in advance for this webinar: https://zoom.us/webinar/register/WN_3YbVuQHIQ4m4MZYw7svSqQ After registering, you will receive a confirmation email containing information about joining the webinar. Should you not be able to join the Webinar, the Colloquium is also available in live streaming at: ictp.it/livestream. The Lecture Series takes place on 27, 28 and 29 January 2021 at 16.00 hrs each day on the same Zoom ID. The Abdus Salam Distinguished Lecture Series receives generous support from the Kuwait Foundation for the Advancement of Sciences (KFAS). For more information see: https://kfas.ictp.it/ ICTP pio@ictp.it

Seminar

Mathematics

ICTP/SISSA Math Seminar on Kähler Geometry: Title to be announced

Speaker: Michael Hallam (Oxford University)

Seminar Start Time: 14:00

Seminar

11 Feb 2021

@ Zoom Meeting

Strings and Higher Dimensional Theories

Null Boundary Charges and Symmetries

Speaker(s): Shahin Sheikh Jabbari (IPM, Tehran, Iran)

Abstract. Formulation of theories with local symmetries in presence of boundaries has revealed interesting features, stressing further the significance of "boundary degrees of freedom" (b.d.o.f.) and the symmetries and algebras arranging the b.d.o.f. In particular, one may apply these ideas to black hole solutions to gravity theories where the horizon can be viewed as a null boundary for the set of observers outside the horizon. The b.d.o.f. and the associated charges and algebras in these examples may remedy problem of identification of black hole microstates. In this talk I provide a general discussion on the formulation of null boundary symmetries and algebras and summarise and the latest developments in realisation of the Hawking-Perry-Strominger idea.

Seminar Start Time: 14:30

Europe/Rome Please register in advance for this meeting at: https://zoom.us/meeting/register/tJcvdu6vpzwvEtMOgmJk_-8hVI20cRrXsZ9O After registering, you will receive a confirmation email containing information about joining the meeting. Zoom Meeting ICTP pio@ictp.it

Seminar

18 Feb 2021

@ Zoom Meeting

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Speaker(s): Ben Freivogel (University of Amsterdam)

Seminar Start Time: 14:30

Seminar

23 Feb 2021

@ Zoom Meeting

Cosmology

HECAP Seminar: Title to be announced

Speaker(s): Valerie Domcke (CERN)

Seminar Start Time: 14:30

Europe/Rome Perhaps the most promising candidate for a source of H2 in future hydrogen driven global energy economy is the electrolytic splitting of H2O. For the reductive half of this reaction, i.e. the hydrogen evolution reaction (HER), Pt is the current champion catalyst and its cost and scarcity limit widespread deployment of devices based on this chemistry. The HER on Pt has been studied for decades and, for much of that time, an enormous amount of effort has been expended looking for alternative catalysts with similar activity and stability, largely without success. Part of the challenge of such materials discovery efforts is that why Pt is such an excellent HER catalyst is not well understood: there is no proposed HER mechanism that is consistent with all experimental observations (e.g. that can explain the dependence on electrolyte, Pt surface structure and pH). Experimentally characterising HER mechanism is challenging: measurements under steady-state nonequilibrium conditions cannot generally distinguish intermediates from unwanted side products and elementary processes with timescales of femtoseconds to seconds are all important in understanding reactivity. We approach this problem by performing perturbation experiments in which we alter the chemical potential of Pt electrons using a femtosecond optical pulse and monitor interfacial structure using a combination of femtosecond resolved electrical and optical techniques as the electronic excitation dissipates. In this talk I will show how experiments detecting femtosecond induced photocurrents suggest that charge transfer along the Pt-H bond can be inhibited by interfacial water structure, how the results of interface-specific vibrational spectroscopy suggest that adsorbed hydrogen readily diffuses between different types of atop adsorption sites, and how this mobility appears to dramatically change at 0 V vs. RHE. Virtual ICTP pio@ictp.it

Seminar

24 Feb 2021

@ Virtual

HECAP Seminar: Title to be announced

Speaker(s): Michele Del Zotto (Uppsala University, Sweden)

Seminar Start Time: 14:30

Seminar

22 Apr 2021

@ Zoom Meeting

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Speaker(s): Mark Van Raamsdonk (University of British Columbia)

Seminar Start Time: 17:00

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Virtual Seminars

Seminar

Condensed Matter and Statistical Physics

CMSP Seminar (Joint ICTP/SISSA Statistical Physics): The Topography of Random Surfaces: Percolation Transitions and Conformal Fractals

Ceremony

GRADUATION CEREMONY: Master of Advanced Studies in Medical Physics (2019/2020)

Seminar

Salam Distinguished Lectures 2021 by Prof. David Spergel. Lecture 1: "What the Universe’s Baby Picture Reveals About Fundamental Physics"

Seminar

Salam Distinguished Lectures 2021 by Prof. David Spergel: Lecture 2: “Our Simple Strange Universe”

Ceremony

2019 Dirac Medal and Prize Ceremony

Seminar

Mathematics

ICTP/SISSA Math Seminar on Kähler Geometry: Optimal symplectic connections and stability of fibrations

Seminar

Salam Distinguished Lectures 2021 by Prof. David Spergel: Lecture 3: "Determining the Universe’s Initial Conditions”

Seminar

Condensed Matter and Statistical Physics

CMSP Seminar (Joint ICTP/SISSA Statistical Physics): To be announced

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Mathematics

ICTP/SISSA Math Seminar on Kähler Geometry: Title to be announced

Seminar

Strings and Higher Dimensional Theories

Null Boundary Charges and Symmetries

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Cosmology

HECAP Seminar: Title to be announced

Seminar

Condensed Matter and Statistical Physics

CMSP Seminar (Atomistic Simulation Webinar Series): Towards an Experimental, Femtosecond-resolved, view of Hydrogen Evolution on Platinum

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Phenomenology of Particle Physics

HECAP Seminar: Title to be announced

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Cosmology

HECAP Seminar: Title to be announced

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

Seminar

Strings and Higher Dimensional Theories

HECAP Seminar: Title to be announced

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