Events

Upcoming
15
FEB
2026
SCHOOL OF PARTICLES AND ACCELERATORS
Special Seminar / Virtual Format
Precision Flavour Physics as a Probe of New Physics

SCHOOL OF PARTICLES AND ACCELERATORS

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Special Seminar / Virtual Format
Precision Flavour Physics as a Probe of New Physics

Dr. Siavash Neshatpour, Universit´e Claude Bernard Lyon 1, France


15 FEB 2026
11:00 - 12:30

Rare flavour-changing processes provide some of the most sensitive probes of physics beyond the Standard Model, often accessing energy scales far above the direct reach of current colliders. Fully exploiting this sensitivity requires precise theoretical control over both short-distance dynamics and long-distance hadronic effects. This talk discusses recent progress in rare B- and K-meson decays aimed at strengthening the theoretical foundations needed to turn precision measurements into robust tests of the Standard Model.
In rare $b\to s\ell\ell$ transitions, persistent tensions with Standard Model predictions motivate model-independent global analyses of current data. These studies systematically assess theoretical uncertainties, with particular emphasis on nonlocal hadronic contributions that can mimic signals of new physics. Data-driven approaches based on analyticity and unitarity, together with first-principles calculations using light-cone sum rules and dispersive methods, provide complementary strategies to disentangle hadronic effects from genuine short-distance contributions, enabling consistent effective-field-theory interpretations and translating precision measurements into quantitative constraints on high-scale new physics.
Rare kaon decays offer an independent and complementary laboratory, where long-distance dynamics play a more prominent role but can be brought under control. New constraints on vector, axial-vector, scalar, and pseudoscalar interactions from charged- and neutral-lepton modes are also highlighted, alongside improved non-perturbative inputs from global analyses of $K \to 3\pi$ data, with implications for ongoing and future high-intensity kaon experiments.



Indico Link: https://indico.hep.ipm.ir/e/Neshatpour


Meeting Place: Virtual Format


Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/special-seminar


Link: https://indico.hep.ipm.ir/e/Neshatpour
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17
FEB
2026
SCHOOL OF PARTICLES AND ACCELERATORS
The 5th Workshop on
Experimental Particle Physics

SCHOOL OF PARTICLES AND ACCELERATORS

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The 5th Workshop on
Experimental Particle Physics

List of Speakers - School of Particles and Accelerators, IPM, Tehran


17 FEB 2026
09:00 - 17:00

Abstract:

With over two decades of active involvement in experimental particle physics, particularly through the CMS experiment at CERN, the School of Particles and Accelerators is pleased to present the 5th IPM Workshop on Experimental Particle Physics. This one-day event will provide an in-depth introduction to the core concepts, methods, and tools used in experimental particle physics.

The workshop is designed to engage graduate students, post-doctoral researchers, and faculty members in exploring the various areas of this dynamic field. Attendees will have the opportunity to gain valuable insights into the latest developments and applications in particle physics research.

This year's workshop will focus on the following topics:
• Introduction to Experimental Particle Physics
• High-Energy Physics Detectors Systems
• Tools for Physics Data Analysis
• Methods of Data Analysis in Particle Physics


Februray 17, 2026


Meeting Place:
Seminar Room, School of Particles and Accelerators, IPM

5th Workshop School Page:
https://particles.ipm.ir/conferences/2026/hep-exp/index.jsp


Link: https://particles.ipm.ir/conferences/2026/hep-exp/index.jsp
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17
FEB
2026
SCHOOL OF PHYSICS
Weekly Seminar
HEPCo Group
WIMP Meets ALP: Coherent Freeze-Out of Dark Matter

SCHOOL OF PHYSICS

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Weekly Seminar
HEPCo Group
WIMP Meets ALP: Coherent Freeze-Out of Dark Matter

B. Yu, Cornell University


17 FEB 2026
14:00 - 15:00

Date and time

Tuesday,ِ February 17, 2026 (28 Bahman 1404), 7:00 pm Tehran time/ 10:30 AM EST




Link

https://www.skyroom.online/ch/schoolofphysics/highenergyseminar


Abstract

The microscopic nature of dark matter is the major open question in science. Weakly Interacting Massive Particles (WIMPs) and Axion-Like Particles (ALPs) are the two most theoretically motivated dark matter candidates. Thousands of papers consider them separately. We point out that if both species are present in the theory, even a tiny (Planck-suppressed) interaction between them can lead to drastic modifications of their dynamics in the early universe. This can dramatically change predicted properties of WIMP and ALP dark matter particles, such as their masses and annihilation cross sections. This in turn leads to important consequences for experiments searching for particle dark matter.

Link: https://www.skyroom.online/ch/schoolofphysics/highenergyseminar
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18
FEB
2026
SCHOOL OF PARTICLES AND ACCELERATORS
Joint Astronomy & Particle Physics Colloquium - Hybrid Format
Extra-terrestrial neutrinos as a window towards new physics

SCHOOL OF PARTICLES AND ACCELERATORS

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Joint Astronomy & Particle Physics Colloquium - Hybrid Format
Extra-terrestrial neutrinos as a window towards new physics

Dr. Yasaman Farzan, School of Physics, IPM


18 FEB 2026
12:30 - 13:30

The current neutrino telescopes, ICECUBE and KM3NeT, have ushered in a new era for the fields of particle physics and astrophysics, bringing these two communities closer together and urging further dialogue between these fields. I will start with a short review of the possible sources of extra-terrestrial neutrinos. I will then review the results from these telescopes as well as the prospect of their upgrade and construction of new neutrino telescopes. I will emphasize the serendipity nature of research in this field, with the frenzy of activity following the famous KM3-230213A event as an example. In the end, I will briefly review our paper explaining this unusual and unexpected event which defies a standard model explanation.



Indico Link:https://indico.hep.ipm.ir/e/Y.Farzan


Meeting Place: Seminar Room, School of Particles and Accelerators, IPM


Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/special-seminar


Link: https://indico.hep.ipm.ir/e/Y.Farzan
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18
FEB
2026
SCHOOL OF MATHEMATICS
Combinatorics and Computing Weekly Seminar
Sharp Thresholds for Spanning Regular Subgraphs

SCHOOL OF MATHEMATICS

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Combinatorics and Computing Weekly Seminar
Sharp Thresholds for Spanning Regular Subgraphs

Maksim Zhukovskii, University of Sheffield, England


18 FEB 2026
14:00 - 15:00

A graph property is called increasing if it is closed under addition of edges. For an increasing property, the probability of its occurrence in the binomial random graph G(n,p) transitions rapidly (in asymptotics) from 0 to 1 as p crosses the so-called probability threshold. Since the original paper of Erdos and Renyi the task of determining the asymptotic behaviour of threshold probabilities for increasing properties has been a central topic in probabilistic combinatorics. While the asymptotic order of the probability threshold has been determined for many natural increasing graph properties, a general solution remains unknown, and determining the exact asymptotics is even more challenging. In the talk I will provide an answer to the latter question for a class of increasing properties generated by d-regular graphs. This family of d-regular graphs contains asymptotically almost all d-regular graphs and, in particular, it contains the square of a cycle. This resolves a conjecture of Kahn, Narayanan, and Park, regarding the asymptotics of the threshold for the appearance of the square of a Hamilton cycle.
Zoom room information:
https://us06web.zoom.us/j/86247043799?pwd=KH1lKfYt1rGLzSgKk31MwprllTiOef.1
Meeting ID: 862 4704 3799
Passcode: 362880

Venue: Niavaran, Khosrovshahi Lecture Hall

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18
FEB
2026
SCHOOL OF MATHEMATICS
Geometry and Topology Weekly Seminar
On the Geometrization and Epigenetics of Mathematics.

SCHOOL OF MATHEMATICS

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Geometry and Topology Weekly Seminar
On the Geometrization and Epigenetics of Mathematics.

Esmail Arasteh, IPM


18 FEB 2026
15:30 - 17:00

Deep ideas silently reappear across diverse fields of mathematics. They shape nature. Determine which questions are natural to be asked, which objects are fundamental, what is a meaningful equivalence, etc. Many phenomena are deeply rooted in their essence. In this talk, we try to recall some of these metaphorical ideas. We will discuss some examples of geometrization (resp. categorification/decategorification) process, including Hecke stacks and Hecke operators.
Venue: Niavaran, Khosrovshahi Lecture Hall

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Past
10
FEB
2026
SCHOOL OF ASTRONOMY
Weekly Seminar
Detection of quadruple structure near the ASCC 32 region via machine learning methods

SCHOOL OF ASTRONOMY

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Weekly Seminar
Detection of quadruple structure near the ASCC 32 region via machine learning methods

Mohammad Noormohammadi
(IPM)


10 FEB 2026
11:00 - 13:00

Multiple structures within stellar groups are an intriguing subject for theoretical and observational studies of stellar formation. With the accuracy and completeness of data from Gaia Data Release 3, we now have new opportunities to detect reliable members of stellar groups across a larger field of view than in previous studies. In this work, using machine learning methods and high-accuracy data, we investigate the possibility of detecting multiple structures within 500 arcmin of ASCC 32. We first applied DBSCAN to proper motion and parallax, as multiple structures tend to share similar values for these parameters. Next, we applied GMM to position, proper motion, and parallax for the members detected by DBSCAN. This approach allowed us to identify a filamentary structure among the DBSCAN-detected members. This structure contains all stellar groups previously identified in this region. Subsequently, based on the BIC score, we applied GMM to this filamentary structure. Since multiple structures exhibit distinct positional distributions, GMM was able to effectively separate all groups within the filament. Our methods successfully identified ASCC 32, OC 0395, and HSC 1865 within a 500 arcmin radius. Additionally, we found two distinct substructures within ASCC 32. These four groups exhibit a single main-sequence distribution in the CMD, with proper motion values within three times the standard deviation and slightly differing parallax values, despite having distinct spatial structures. Furthermore, these four groups share the same radial velocity distribution. We provide documentation demonstrating the formation of these stellar groups as a multiple structure, with improved membership identification compared to previous studies.

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10
FEB
2026
SCHOOL OF PHYSICS
Weekly Seminar
HEPCo Group
Scaling Symmetry and Carrollian Gravity

SCHOOL OF PHYSICS

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Weekly Seminar
HEPCo Group
Scaling Symmetry and Carrollian Gravity

M. Ahmadi-Jahmani, Ferdowsi University of Mashhad


10 FEB 2026
14:00 - 15:00

Date and time

Tuesday,ِ February 10, 2026 (21 Bahman 1404), 2:00 pm (Tehran time)




Link

https://www.skyroom.online/ch/schoolofphysics/highenergyseminar


Abstract

In this presentation, we formulate matter-coupled scaling-Carroll gravity as a gauge theory and analyze its associated gravity multiplet. After fixing the scaling symmetry, the theory is governed by the trace of the extrinsic curvature, the Carroll boost symmetry, and a vector field derived from dilatation. We demonstrate that appropriate gauge choices and geometric constraints lead to distinct regimes, including dynamical Carroll gravity, Aristotelian gravity, and a fracton gauge theory coupled to Aristotelian geometry. In the fracton phase, the Carroll boost parameter functions as a vector-charge gauge symmetry.

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3
FEB
2026
SCHOOL OF ASTRONOMY
Weekly Seminar
Geometry of non-Gaussianity in transient non-attractor inflation

SCHOOL OF ASTRONOMY

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Weekly Seminar
Geometry of non-Gaussianity in transient non-attractor inflation

Bahar Nikbakht
(IPM)


3 FEB 2026
11:00 - 13:00

Inflationary models with a transient non-attractor phase are interesting because they can produce primordial black holes (PBHs) and scalar-induced gravitational waves (SIGWs). These models are usually studied using only their power spectrum. In this talk, we argue that this is not enough, and non-Gaussianities play a crucial role. In particular, we show that non-linear effects can change not only the abundance of PBHs and the amplitude of SIGWs, but also their mass and frequency distributions. First, we extend the single-field consistency relation to cases where scale invariance is strongly broken. We find that the peak of squeezed-limit non-Gaussianity does not coincide with the peak of the power spectrum. As a result, the scales relevant for PBH formation and SIGW production can be shifted or extended compared to linear predictions. We then study the geometry — i.e., the shape and scale —of the full bispectrum. Near the peak of the power spectrum, we find that the equilateral configuration dominates over the squeezed one. We then introduce a simple scale-dependent, local-like estimator that captures the main features of the full bispectrum. Finally, we find that considering the full bispectrum shifts and extends the scales of the PBHs, as was predicted primarily by the squeezed limit. Our results show that a full non-Gaussianity analysis is necessary for reliable predictions of PBHs and SIGWs in these models.



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3
FEB
2026
SCHOOL OF PHYSICS
Weekly Seminar
HEPCo Group
How light can ALP dark matter?

SCHOOL OF PHYSICS

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Weekly Seminar
HEPCo Group
How light can ALP dark matter?

K. Chathirathas, Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT)


3 FEB 2026
14:00 - 15:00

Date and time

Tuesday, February 3rd, 2026 (14 Bahman 1404), 2:00 pm (Tehran time)




Link

https://www.skyroom.online/ch/schoolofphysics/highenergyseminar


Abstract

I discuss lower bounds on the mass of axion-like particles, assuming they make up all of dark matter. Distinguishing between pre- and post-inflationary symmetry breaking, I identify the allowed parameter space in terms of the axion mass and the inflationary energy scale. In the post-inflationary scenario, recent simulations show that axion radiation from cosmic strings dominates dark matter production, leading to significantly weaker isocurvature constraints than previously thought. Combining these with limits from black hole superradiance and free streaming yields a generic bound ma≳10^{−17} eVm_a \gtrsim 10^{-17}\,\mathrm{eV}, with possible relaxation in specific scenarios. I also show that the absence of CMB tensor modes can impose much stronger bounds, reaching ma≳5×10 ^{−17}   eVm_a \gtrsim 5 \times 10^{-7}\,\mathr for low reheating efficiencies.



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27
JAN
2026
SCHOOL OF PHYSICS
Weekly Seminar
HEPCo Group
Weak Decays of the Omega_{b}^{*} Baryon and Their Role in Its Experimental Establishment

SCHOOL OF PHYSICS

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Weekly Seminar
HEPCo Group
Weak Decays of the Omega_{b}^{*} Baryon and Their Role in Its Experimental Establishment

A. Amiri, Ferdowsi University of Mashhad


27 JAN 2026
14:00 - 15:00

Date and time

Tuesday,ِ January 13th, 2026 (23 Dey 1404), 2:00 pm (Tehran time)




Link

https://www.skyroom.online/ch/schoolofphysics/highenergyseminar


Abstract

The spin-3/2 ground-state bottom baryon \Omega^{*}_{b} remains one of the least explored members of the heavy-baryon spectrum. Owing to the absence of any Okubo-Zweig-Iizuka (OZI)-allowed strong decay channels, together with the presence of a soft photon in its radiative decay, experimental establishment of \Omega^{*}_{b} is particularly challenging. In this talk, we present a detailed study of the weak decays of \Omega^{*}_{b} as a promising pathway toward its experimental establishment. We analyze both semileptonic and nonleptonic weak decays of the transition \Omega^{*}_{b} --> \Omega^{*}_{c}, treating them within a unified theoretical framework. First, the transition form factors governing this heavy-to-heavy baryonic process are calculated using the QCD sum rule approach, ensuring consistency with Lorentz invariance and the spin- 3/2 nature of the participating baryons. These form factors are then employed to compute decay amplitudes, and decay widths for the semileptonic channels \Omega^{*}_{b} \Omega^{*}_{c} --> \ell\bar{\nu}_{\ell} and nonleptonic transitions \Omega^{*}_{b}--> \Omega^{*}_{c}M, where M denotes a pseudoscalar or vector meson. Taken together, the results demonstrate that weak decay modes provide a coherent and realistic strategy for the experimental identification of the \Omega^{*}_{b} baryon at current and future hadron experiments.

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25
JAN
2026
SCHOOL OF PARTICLES AND ACCELERATORS
4th Advanced School on
Holography and Quantum Information Topics (2-day)

SCHOOL OF PARTICLES AND ACCELERATORS

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4th Advanced School on
Holography and Quantum Information Topics (2-day)

List of Speakers - School of Particles and Accelerators, IPM, Tehran


25 JAN 2026
09:00 - 17:00

Abstract:

In recent years, exciting connections have emerged between quantum information theory, quantum gravity, and quantum many-body systems, reshaping our understanding of fundamental physics. To explore these developments and foster deeper interdisciplinary links, the School of Particles and Accelerators at IPM has launched an ongoing series of workshops. These events bring together experts and young researchers to review recent progress, exchange ideas, and strengthen collaborations between the quantum information and high-energy physics communities.

January 24-25, 2026


Meeting Place:
Seminar Room, School of Particles and Accelerators, IPM

4th Advanced School Page:
https://particles.ipm.ir/conferences/2026/shqi/index.jsp


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24
JAN
2026
SCHOOL OF PARTICLES AND ACCELERATORS
4th Advanced School on
Holography and Quantum Information Topics (2-day)

SCHOOL OF PARTICLES AND ACCELERATORS

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4th Advanced School on
Holography and Quantum Information Topics (2-day)

List of Speakers - School of Particles and Accelerators, IPM, Tehran


24 JAN 2026
09:00 - 17:00

Abstract:

In recent years, exciting connections have emerged between quantum information theory, quantum gravity, and quantum many-body systems, reshaping our understanding of fundamental physics. To explore these developments and foster deeper interdisciplinary links, the School of Particles and Accelerators at IPM has launched an ongoing series of workshops. These events bring together experts and young researchers to review recent progress, exchange ideas, and strengthen collaborations between the quantum information and high-energy physics communities.

January 24-25, 2026


Meeting Place:
Seminar Room, School of Particles and Accelerators, IPM

4th Advanced School Page:
https://particles.ipm.ir/conferences/2026/shqi/index.jsp


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21
JAN
2026
SCHOOL OF MATHEMATICS
Mathematics Colloquium
Radition Damping and Stability of Stationary Solutions of Nonlinear Wave Equations.

SCHOOL OF MATHEMATICS

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Mathematics Colloquium
Radition Damping and Stability of Stationary Solutions of Nonlinear Wave Equations.

Sohrab Shahshahani , .


21 JAN 2026
16:00 - 17:00

In this expository talk I will describe a nonlinear mechanism for the stability of time-independent solutions of certain nonlinear wave equations. This mechanism, known as radition damping, stems from the interaction between the discrete and continuous spectra of the underlying linear operator. I will first present a fews classical examples where stability fails at the linear level, and then explain how radiation damping restores stability for the full equation.
Good references for the material I will discuss include:
-A. Soffer and M.I. Weinstein: Invent. Math. 136 (1999), no. 1, 9-74
-D. Bambusi and S. Cuccagna: Amer, J. Math. 133(2011), no. 5, 1421-1468
Venue: Niavaran, Khosrovshahi Lecture Hall

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7
JAN
2026
SCHOOL OF PARTICLES AND ACCELERATORS
Wednesday Weekly Seminar - Hybrid Format
Improved Constraints on Pion Fragmentation Functions from Simulated Electron-Ion Collider Data

SCHOOL OF PARTICLES AND ACCELERATORS

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Wednesday Weekly Seminar - Hybrid Format
Improved Constraints on Pion Fragmentation Functions from Simulated Electron-Ion Collider Data

Dr. Majid Azizi - School of Particles and Accelerators, IPM


7 JAN 2026
11:00 - 12:00

Abstract:

I present a quantitative study of how future Electron–Ion Collider (EIC) semi-inclusive DIS (SIDIS) measurements can improve the determination of parton-to-pion fragmentation functions. Using an NLO pQCD framework with a neural-network parametrization and Monte Carlo uncertainty propagation, we perform two global fits: (i) existing SIA and SIDIS data (HERMES and COMPASS), and (ii) the same dataset augmented by EIC SIDIS pseudo-data at. The pseudo-data are generated consistently within the same NLO collinear-factorization framework, with realistic statistical and correlated systematic uncertainties. We find that including EIC pseudo-data leads to a substantial reduction of fragmentation-function uncertainties, most notably at medium-to-large z, with particularly strong gains for selected light-quark channels and a clear improvement for the gluon fragmentation function.


Indico Link:
https://indico.hep.ipm.ir/e/M.Azizi1

Meeting Place:
Seminar Room, School of Particles and Accelerators, IPM

Link to Join Virtually:
https://www.skyroom.online/ch/ipm-particles/weekly-seminar

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7
JAN
2026
SCHOOL OF QUANTUM PHYSICS AND MATTER
QPM Weekly Seminar (Hybrid Format)
Landau levels and low-energy k.p effective Hamiltonian of 2D topological insulator: Ruthenium and Osmium Carbide (OsC, RuC) in monolayer hexagonal structure

SCHOOL OF QUANTUM PHYSICS AND MATTER

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QPM Weekly Seminar (Hybrid Format)
Landau levels and low-energy k.p effective Hamiltonian of 2D topological insulator: Ruthenium and Osmium Carbide (OsC, RuC) in monolayer hexagonal structure

Hadi Khanjani


7 JAN 2026
14:00 - 15:00

The distinctive properties of two-dimensional topological insulators have driven significant interest in discovering new materials of them with unique mechanical, electrical, thermal, and optical characteristics. Among the promising candidates are Ruthenium Carbide (RuC) and Osmium Carbide (OsC) in a hexagonal structure, whose room-temperature stability has been confirmed through computational studies. In this talk, I will begin by introducing two-dimensional topological insulators. Next, I will demonstrate how effective low-energy Hamiltonians for these systems can be derived from crystal symmetries using k.p theory. Finally, I will examine their behavior under an applied magnetic field.




Venue: Room D, 3rd Floor, Farmanieh Building, IPM
Link: https://vmeeting2.ipm.ir/b/nan-gkn-wmh-exh

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7
JAN
2026
SCHOOL OF BIOLOGICAL SCIENCES
School of Biological Science
Cancer as an Evolutionary Process

SCHOOL OF BIOLOGICAL SCIENCES

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School of Biological Science
Cancer as an Evolutionary Process

Dr. Javad Mowla


7 JAN 2026
15:00 - 16:00

Cancer is increasingly understood as an evolutionary process, shaped by the principles of mutation, selection, and adaptation. Tumor cells form heterogeneous populations that compete for resources and survival, undergoing clonal expansion when advantageous genetic or epigenetic changes arise. This Darwinian dynamic explains the emergence of hallmark traits such as uncontrolled proliferation, resistance to therapy, and metastatic potential. Beyond genetic instability, non-genetic mechanisms - including epigenetic reprogramming and interactions with the tumor microenvironment - further drive diversification and adaptation. Viewing cancer through an evolutionary lens not only clarifies its complexity but also highlights new strategies for intervention, emphasizing the need to anticipate and steer tumor evolution rather than merely react to it.

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6
JAN
2026
SCHOOL OF ASTRONOMY
Weekly Seminar
Large-scale cosmic anomalies: current status, future prospects, and possible explanations

SCHOOL OF ASTRONOMY

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Weekly Seminar
Large-scale cosmic anomalies: current status, future prospects, and possible explanations

Yashar Akrami
(UAM)


6 JAN 2026
11:00 - 13:00

Even though the current observational data show an extremely high level of agreement with predictions of the standard model of cosmology, LambdaCDM, the cosmic microwave background (CMB) temperature fluctuations measured by the WMAP and Planck satellites have shown a number of persistent anomalous features on large-angular scales that are unexpected or extremely unlikely in LambdaCDM cosmology. These anomalies, which are properties of the observed sky and not instrumental artifacts, are all related to violation of statistical isotropy, and even though they could, individually taken, be statistical flukes, they may also be hints of new physics beyond the standard cosmological model. In this talk, after providing a critical review of the CMB large-angular-scale anomalies, their history, and their current status, I will discuss some of the existing explanations for the features, ranging from the fluke hypothesis and astrophysical foregrounds within LambdaCDM to different physical models beyond the standard picture, in particular the possibility that the Universe has a non-trivial topology, and will review phenomenological expectations for each explanation. I will argue that, in addition to the new perspectives on existing data that the powerful and continuously advancing computational and statistical techniques may provide, it is also essential to investigate the anomalies further with upcoming and future high-precision cosmological data, including observations of the CMB polarization and the cosmic large-scale structure. This is because any observations of similar or related anomalies in any data sets other than the CMB temperature sky will ameliorate concerns about look-elsewhere penalties for the a posteriori statistical characterization of the CMB temperature anomalies while dramatically increasing the statistical significance of the features to a level which will inevitably force us to revise or rethink the standard model of cosmology.

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News

Joint Astronomy and Particle Physics Colloquium
Extra-terrestrial neutrinos as a window towards new physics
Yasaman Farzan, School of Physics, IPM
Wednesday, Feb 18, 2026 - 12:30
Breakthrough Prize in Fundamental Physics 2025 Awarded to the CMS Collaboration
This recognition reflects years of dedicated scientific, technical, and operational contributions by the IPM CMS team to CERN.
The 5th Workshop on Experimental Particle Physics
Februray 17, 2026 (28 Bahman 1404)
Akhbar 114: Fall 2024
New Issue of IPM Newsletter, "Akhbar"
School of Biological Sciences Colloquium
Cancer as an Evolutionary Process
Dr. Javad Mowla
07 JAN 2026, 15:00
Call for establishment in the innovation center of IPM
School of Biological Sciences Colloquium
What are we doing as scientists in Iran?
Reza Mansouri
31 Dec 2025, 15:00
School of Biological Sciences Colloquium
Global Warming: Causes and Solutions
Yousef Sobouti, IASBS
24 Dec 2025, 15:00
Paper Published in Nature Human Behaviour
Dr. Mehdi Sanayei
School
National School on Quantum Information Science


Scientific news in the media

Neutrinos, Theory, and Women in Physics
Yasaman Farzan, Simons Associate at ICTP, discusses her life and work
(An interview with ICTP)

 A project to boost study of human brain

 The Culture of Research and Scholarship in Mathematics



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