Grant: Subatomic Physics Envelope - Individual
Concordia University
$90,000.00
Beyond the Standard Model Scenarios: Dark Matter and Collider Signals
FY 2024-25
Summary
The Standard Model of Particle Physics is one of the most successful scientific theories in history. It can explain a wide range of subatomic phenomena in terms of a few symmetry principles and a handful of constants of nature. There are however, very good reasons to believe that the Standard Model is not the final answer to questions about the fundamental structure of matter. On one hand, there are theoretical concerns about the tuning of the parameters in the model. On the other hand, experimental evidence such as the neutrino flavour oscillations and the existence of dark matter (crucial for the formation of galaxies) remains unexplained in the Standard Model.
It is widely believed that the solution to these puzzles requires the existence of new particles and/or new interactions. Unfortunately, although many predictions of beyond the Standard Model physics are available, no conclusive proof of new particles or interactions exists. There are two possible explanations as to why new particles may have escaped detection so far. First, they could be too heavy to be produced in current experiments. Most of my research has been concentrated so far on this idea, and in part of my new research project, I would like to revisit this possibility, and perform a careful study of the assumptions involved (using newly developed software), with the purpose of widening the parameter space still available for new particles and new interactions. A second possibility is that the new particles are hidden, because they couple so feebly to ordinary matter. It may be that the rate at which they are produced is too small, or alternatively, that they form a compressed spectrum, that is, one which does not easily yield observed signals. In this case, the most promising strategy would be to make more precise measurements, and to increase the number of events in experiments (intensity frontier) to find them. I propose to devise some searches at the LHC by choosing observables with little interference from the background, and complimentary to searching in proton-proton collisions, to look for these particles in heavy ion collisions.
Program
Subatomic Physics Envelope - Individual
Recipient
Location
Quebec, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
SAPIN-2020-00036
Name nom
Frank, Mariana
Department département
Physics - Physics
Organization id
70
Institution établissement
Concordia University
Province en
Québec
Province fr
Québec
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2024
Competition year année de concours
2020
Award amount
90000
Program id
SAPIN
Program name en
Subatomic Physics Envelope - Individual
Program name fr
Enveloppe de physique subatomique - Individuelles
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR LA DÉCOUVERTE
Committee code
19
Committee name en
Subatomic Physics
Committee name fr
Physique subatomique
Area of application code
1202
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Physical sciences
Area of application fr
Sciences physiques
Research subject code
3104
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Particle physics
Research subject fr
Physique des particules
Field of research list names en
Not available
Field of research list names fr
Non disponible
Socioeconomic objective list names en
Not available
Socioeconomic objective list names fr
Non disponible
Application title
Beyond the Standard Model Scenarios: Dark Matter and Collider Signals
Keywords
supersymmetry; left-right models; dark matter; u(1)' models; additional fermions or bosons; weak interactions
Application summary
The Standard Model of Particle Physics is one of the most successful scientific theories in history. It can explain a wide range of subatomic phenomena in terms of a few symmetry principles and a handful of constants of nature. There are however, very good reasons to believe that the Standard Model is not the final answer to questions about the fundamental structure of matter. On one hand, there are theoretical concerns about the tuning of the parameters in the model. On the other hand, experimental evidence such as the neutrino flavour oscillations and the existence of dark matter (crucial for the formation of galaxies) remains unexplained in the Standard Model.
It is widely believed that the solution to these puzzles requires the existence of new particles and/or new interactions. Unfortunately, although many predictions of beyond the Standard Model physics are available, no conclusive proof of new particles or interactions exists. There are two possible explanations as to why new particles may have escaped detection so far. First, they could be too heavy to be produced in current experiments. Most of my research has been concentrated so far on this idea, and in part of my new research project, I would like to revisit this possibility, and perform a careful study of the assumptions involved (using newly developed software), with the purpose of widening the parameter space still available for new particles and new interactions. A second possibility is that the new particles are hidden, because they couple so feebly to ordinary matter. It may be that the rate at which they are produced is too small, or alternatively, that they form a compressed spectrum, that is, one which does not easily yield observed signals. In this case, the most promising strategy would be to make more precise measurements, and to increase the number of events in experiments (intensity frontier) to find them. I propose to devise some searches at the LHC by choosing observables with little interference from the background, and complimentary to searching in proton-proton collisions, to look for these particles in heavy ion collisions.