High Energy and Computational Physics

 

Our research interests involve theoretical and experimental high energy, particle and astro-particle physics, cosmology, physics of inflation and early Universe, in particular gravitational waves.

The lab has over 20 scientists from over six different countries. We are part of the CMS collaboration at CERN and of the LISA gravitational wave detector collaboration at the European Space Agency (ESA). We work to determine the fundamental nature of the universe through gravitational waves and other physics in the centre of excellence „Foundations of the  Universe“ in collaboration with the University of Tartu and Tallinn Technical University.

The computing centre of the laboratory has a powerful cluster with 6000 cores and 4 PB of storage. We do CMS particle physics simulations, compute phase transitions in the early Universe, and other computations that need high performance computing. We take part in the ETAIS to develop the scientific computing infrastructure in Estonia.

Dr. Martti Raidal

Head of Laboratory

Dr. Martti Raidal
Email
CV ORCID Inspire

If you are a student and interested in doing a project or a thesis with us, you might find this page useful.

Follow us on social media: BlueSky, Facebook or X

 

For more information please contact our experimental (exp) and theoretical (th) researchers via mail and find below more detailed pages about our various research topics:

 

CMS Trigger Development (EXP)
Machine Learning (EXP)
Gravitational Waves (TH)

 

Latest posts by @kbfihepsocial!

 

#NewPaper from M. Lewicki (U. of Warsaw), P. Toczek (U. of Warsaw) and V. Vaskonen (KBFI) about primordial #blackholes and #gravitationalwaves from early universe phase transitions: arxiv.org/abs/2412.10366. [1/3]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:24 PM

Ville: We showe that realistic particle physics models can predict first-order phase transitions in the early universe that lead to the formation of primordial black holes with a distinguishable gravitational wave signature that is detectable with future observatories. [2/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:24 PM

Ville: selles töös näitasime, et realistlikud osakestefüüsika mudelid ennustavad esimest järku faasisiirdeid, milles tekivad ürgsed mustad augud ja mille gravitatsioonilainete signaali on võimalik tuleviku observatooriumides avastada. [3/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:24 PM

KBFI is part of the proto-collaboration for the development and realization of Terrestrial Very-Long-Baseline Atom Interferometry (TVLBAI). Several KBFI members contributed to the recent summary of the 2nd TVLBAI workshop: arxiv.org/abs/2412.14960. [1/2]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:20 PM

KBFI osaleb algavas kollaboratsioonis maapealse väga pika baasjoonega aatominterferomeetria (TVLBAI) välja arendamiseks ja teostamiseks. Mitmed KBFI teadlased panustasid hiljutise 2. TVLBAI konverentsi kokkuvõttesse: arxiv.org/abs/2412.14960 [2/2]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:20 PM

#NewResult on #SpaceTime by our theorists Ioannis Gialamas andAntonio Racioppi arxiv.org/abs/2412.17738 [1/3]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:12 PM

Antonio: Allowing space-time to be not only curved but also twisted, symmetry-breaking inflation (an old idea excluded by recent data) becomes viable again. [2/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:12 PM

Antonio: Kui aegruumi saab mitte ainult kõverdada, vaid ka väänata, siis tuleb sümmeetriat rikkuv inflatsioon (vana idee, mille lihtsamad teostused ei ole viimaste andmetega kooskõlas) jälle päevakorda. [3/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) January 9, 2025 at 3:12 PM

#NewResult by our experimentalists Torben Lange and Norman Seeba at the
@cmsexperiment.bsky.social
with a combination of the #CMS LHC Run2 analysis on double #higgs boson production released right in time for Higgs 2025 and this exiting LHC seminar: indico.cern.ch/event/1441587/ #physics [1/3]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) Nov 22, 2024 at 1:42 PM

Torben: This result is an important step in deciphering the Higgs sector and shining light in one of the lesser explored corners of the Standard Model (SM).
We are approaching SMsensitivity fast, and these results promise interesting times are lying ahead. [2/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) Nov 22, 2024 at 1:42 PM

Torben: Meie teadustöö tulemus tähistab olulist edasiminekut Higgsi sektori lahtimõtestamisel ning valgustab seni suhteliselt vähe uuritud piirkonda StandardMudelis. Oleme kiiresti lähenemas SM-i tundlikkuse piirile, ning meie tulemused viitavad, et ees ootavad teaduslikult põnevad ajad. [3/3]

— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) Nov 22, 2024 at 1:42 PM

Non-expert friendly / lihtsas keeles: cms.cern/news/tale-tw… #outreach [3+/3]

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— HEP @ KBFI/NICPB (@kbfihepsocial.bsky.social) December 6, 2024 at 3:59 PM

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