Welcome to TRIUMF!

• Nicole Vassh (TRIUMF)
• Ricky Mizuta (TRIUMF / University of British Columbia)
• Tsung-Han Yeh (TRIUMF)
• Michael Shamma (TRIUMF)
• Carlos Henrique de Lima (TRIUMF)
• Lilianna Hariasz (Queen's University)
• David McKeen (TRIUMF)
• David Morrissey (TRIUMF)
• Douglas Tuckler (TRIUMF and Simon Fraser University)
• Gopolang Mohlabeng (Simon Fraser University and TRIUMF)

Room: Auditorium

Neutrino Mixing from Modular Flavor Symmetries

• Mu-Chun Chen (UC Irvine)

Room: Auditorium

Neutrinos: their origin and their role in the matter-antimatter asymmetry

• Arnab Dasgupta (U Pittsburgh)

Room: Auditorium

Cosmology of Dirac Neutrino Mass Models

• Michael Shamma (TRIUMF)

Room: Auditorium

A low-scale neutrino mass model and energy-dependent oscillation parameters

• Pedro Machado (Fermilab)

Room: Auditorium

Discovering (A) Source of Neutrino Masses at the LHC

• Seyda Ipek

Room: Auditorium

Old Data, New Forensics: The First Second of SN 1987A Neutrino Emission

• Shirley Li (UC Irvine)

Room: Auditorium

Open Discussion Room: Auditorium

Relic neutrinos from collapsars and neutron star mergers

• Liliana Caballero (U Guelph)

Room: Auditorium In highly dense matter scenarios, such as in Supernova, collapsars, and neutron star mergers, neutrinos decouple from matter much earlier and deeper than photons. Their detection in neutrino observatories would allow us to gain valuable insight into the interior, structure, and evolution of these astrophysical environments. While much can be learned from the neutrinos emitted by a single explosion, the rarity of these events combined with neutrinos' weakly interacting nature pose challenges for their detection. Relic neutrinos, emitted since the first Supernovae and mergers occurred in the universe, provide a continuous background flux that offers an additional avenue for the study of matter under strong gravity. In this talk, I shall discuss the diffuse neutrino background from collapsars and neutron star mergers, and the prospects of learning about the equation of state of nuclear matter from its possible detection.

Neutrinos, Collapsars, Neutron Star Mergers, and You: How neutrinos impact heavy element formation in the universe, and the resulting electromagnetic counterpart

• Jonah Miller (Los Alamos)

Room: Auditorium

Probing turbulence in core-collapse supernovae in the upcoming neutrino detectors

• Mainak Mukhopadhyay (Penn State U)

Room: Auditorium

Presupernova Neutrinos: Realistic Emissivities and Detection Possibilities

• Kelly Patton (Trinity College)

Room: Auditorium

P-ONE Neutrino Observatory

• Matthias Danninger (Simon Fraser University)

Room: Auditorium

TRIUMF Colloquium - Core-collapse supernovae as probes of (not only) non-standard neutrino physics

• Anna Suliga (UC Berkely / N3AS)

Room: Auditorium Core-collapse supernovae are one of the most complex phenomena in the Universe. Not only are they one of the production sites of the heavy elements that enable the existence of life, but their cores are also one of the densest environments we can probe, albeit indirectly. Core-collapse supernovae are also among the most spectacular and efficient neutrino factories. Detecting these neutrinos can allow us to probe physics in extreme conditions inaccessible on Earth. In this talk, I will discuss how we can prepare for the next nearby supernova neutrino detection to extract as much information as possible from the neutrino signal. I will also talk about how observing neutrinos from all the past collapses in our Universe – the diffuse supernova neutrino background - can help us better understand the supernova population and may provide hints about physics beyond the Standard Model.

Entaglement of Astrophysical Neutrinos

• Baha Balantekin (U Wisconsin)

Room: Auditorium

Open Discussion Room: Auditorium

Neutrinos vs. Dark Matter

• Kevin Kelly (Texas A&M)

Room: Auditorium

Probes of Neutrinophilc Dark Matter

• Douglas Tuckler (TRIUMF and Simon Fraser University)

Room: Auditorium

Origins of (neutrino-ish) Dark Matter in the Matter Power Spectrum

• Yue Zhang (Carleton U)

Room: Auditorium

The flavour of high-energy neutrinos

• Aaron Vincent (Queen's U)

Room: Auditorium

Neutrinos as standard and nonstandard dark radiation and dark matter

• Kevork Abazajian (UC Irvine)

Room: Auditorium