Abstract: Universal Extra-Dimension models provide a promising framework for model building as they naturally have rich phenomenological implications, not the least of which is a potential natural dark matter candidate. This candidate takes the form of a Kaluza-Klein excitation of some neutral Standard Model field whose stability is ensured by some isometry of the extra-space. In five dimensions, such a symmetry has to be enforced in an ad-hoc fashion, which is why six-dimensional models have started prompting the interest of model builders. If flat 6D models have been thoroughly surveyed and studied, the realm of curved extra-dimensional models remains mostly uncharted. This talk aims at showing the features of extra dimensional models on a curved background, focusing mostly on positively curved spaces. I will show that the main difficulty for constructing a convincing model revolves around the issue of chiral fermions in the 4D effective theory and how it can be overcome by the addition of a new gauge field which has to be hidden from experimental reach by a symmetry breaking. After going over the phenomenological consequences of a model built using these ingredients, I will briefly review hyperbolic extra-dimensions, for which several problems appearing on positively curved spaces are solved or alleviated.
Wits Node Seminar: Dr Sunandan Gangopadhyay (NITheP Stellenbosch)
TITLE: Path integral action of a particle in the noncommutative plane and the Aharonov-Bohm effect
NITheP UKZN Seminar: Prof. Alexander Gorokhov (Samara State University, Russi...Rene Kotze
NITheP UKZN Seminar: Prof. Alexander Gorokhov (Samara State University, Russia)
TITLE: Dynamical Groups, Coherent States and Some of their Applications in Quantum Optics and Molecular Spectroscopy
Wits Node Seminar: Dr Sunandan Gangopadhyay (NITheP Stellenbosch)
TITLE: Path integral action of a particle in the noncommutative plane and the Aharonov-Bohm effect
NITheP UKZN Seminar: Prof. Alexander Gorokhov (Samara State University, Russi...Rene Kotze
NITheP UKZN Seminar: Prof. Alexander Gorokhov (Samara State University, Russia)
TITLE: Dynamical Groups, Coherent States and Some of their Applications in Quantum Optics and Molecular Spectroscopy
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (Uni...Rene Kotze
NITheP WITS node seminar
"Planet Formation in Dense Star Clusters"
to be presented by Dr. Henry Throop (University of Pretoria)
http://www.nithep.ac.za/4hu.htm
NITheP WITS node Seminar by Dr Dr. Roland Cristopher F. Caballar (NITheP/UKZN)
TITLE: "One-Dimensional Homogeneous Open Quantum Walks"
ABSTRACT: In this talk, we consider a system undergoing an open quantum walk on a one-dimensional lattice. Each jump of the system between adjacent lattice points in a given direction corresponds to a jump operator, with these jump operators either commuting or not commuting. We examine the dynamics of the system undergoing this open quantum walk, in particular deriving analytically the probability distribution of the system, as well as examining numerically the behavior of the probability distribution over long time steps. The resulting distribution is shown to have multiple components, which fall under two general categories, namely normal and solitonic components. The analytic computation of the probability distribution for the system undergoing this open quantum walk allows us to determine at any instant of time the dynamical properties of the system.
Stochastic Gravity in Conformally-flat SpacetimesRene Kotze
The National Institute for Theoretical Physics, and the Mandelstam Institute for Theoretical Physics, School of Physics, would like to invite to its coming talk in the theoretical physics seminar series, entitled:
"Stochastic Gravity in Conformally-flat Spacetimes"
to be presented by Prof. Hing-Tong Cho (Tamkang University, Taiwan)
Abstract: The theory of stochastic gravity takes into account the effects of quantum field fluctuations onto the classical spacetime. The essential physics can be understood from the analogous Brownian motion model. We shall next concentrate on the case with conformally-flat spacetimes. Our main concern is to derive the so-called noise kernels. We shall also describe our on-going program to investigate the Einstein-Langevin equation in these spacetimes.
Dates: Tuesday, 17th February 2015
Venue: The Frank Nabarro lecture theatre, P216
Time: 13.20 - 14.10 - TODAY
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (Uni...Rene Kotze
NITheP WITS node seminar
"Planet Formation in Dense Star Clusters"
to be presented by Dr. Henry Throop (University of Pretoria)
http://www.nithep.ac.za/4hu.htm
NITheP WITS node Seminar by Dr Dr. Roland Cristopher F. Caballar (NITheP/UKZN)
TITLE: "One-Dimensional Homogeneous Open Quantum Walks"
ABSTRACT: In this talk, we consider a system undergoing an open quantum walk on a one-dimensional lattice. Each jump of the system between adjacent lattice points in a given direction corresponds to a jump operator, with these jump operators either commuting or not commuting. We examine the dynamics of the system undergoing this open quantum walk, in particular deriving analytically the probability distribution of the system, as well as examining numerically the behavior of the probability distribution over long time steps. The resulting distribution is shown to have multiple components, which fall under two general categories, namely normal and solitonic components. The analytic computation of the probability distribution for the system undergoing this open quantum walk allows us to determine at any instant of time the dynamical properties of the system.
Stochastic Gravity in Conformally-flat SpacetimesRene Kotze
The National Institute for Theoretical Physics, and the Mandelstam Institute for Theoretical Physics, School of Physics, would like to invite to its coming talk in the theoretical physics seminar series, entitled:
"Stochastic Gravity in Conformally-flat Spacetimes"
to be presented by Prof. Hing-Tong Cho (Tamkang University, Taiwan)
Abstract: The theory of stochastic gravity takes into account the effects of quantum field fluctuations onto the classical spacetime. The essential physics can be understood from the analogous Brownian motion model. We shall next concentrate on the case with conformally-flat spacetimes. Our main concern is to derive the so-called noise kernels. We shall also describe our on-going program to investigate the Einstein-Langevin equation in these spacetimes.
Dates: Tuesday, 17th February 2015
Venue: The Frank Nabarro lecture theatre, P216
Time: 13.20 - 14.10 - TODAY
The problem of generating a sequence of true random bits (suitable for cryptographic applications) from random discrete or analog sources is considered. A generalized
version, including Vector Quantization, of the classical approach by Elias for the generation of truly random bits is
introduced, and its performance is analyzed, both in the finite case and asymptotically. The theory allows us to provide an alternative proof of the optimality of the original
Elias’ scheme. We also consider the problem of deriving
random bits from measurements of a Poisson process and
from vectors of iid Gaussian variables. The comparison with
the scheme of Elias, applied to geometric-like non binary
vectors, originally based on the iso-probability property of permutations of iid variables, confirms the potential of the generalized scheme proposed in our work.
Customization of LES turbulence model in OpenFOAMmmer547
This slide is the distribution material on the seminar, "Customization of LES turbulence model in OpenFOAM". (June 13 2015 "OpenCAE Local User Group @ Kansai")
http://ofbkansai.sakura.ne.jp/
Hands on instructions for NITheCS August mini - school Rene Kotze
For all students participating in the NITheCS Mini-School (continuing tomorrow 17 August 2021) - please follow these simple instructions to setup the software environment for the hands-on session for tomorrow.
Francesca Gottschalk - How can education support child empowerment.pptxEduSkills OECD
Francesca Gottschalk from the OECD’s Centre for Educational Research and Innovation presents at the Ask an Expert Webinar: How can education support child empowerment?
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
Instructions for Submissions thorugh G- Classroom.pptxJheel Barad
This presentation provides a briefing on how to upload submissions and documents in Google Classroom. It was prepared as part of an orientation for new Sainik School in-service teacher trainees. As a training officer, my goal is to ensure that you are comfortable and proficient with this essential tool for managing assignments and fostering student engagement.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
June 3, 2024 Anti-Semitism Letter Sent to MIT President Kornbluth and MIT Cor...Levi Shapiro
Letter from the Congress of the United States regarding Anti-Semitism sent June 3rd to MIT President Sally Kornbluth, MIT Corp Chair, Mark Gorenberg
Dear Dr. Kornbluth and Mr. Gorenberg,
The US House of Representatives is deeply concerned by ongoing and pervasive acts of antisemitic
harassment and intimidation at the Massachusetts Institute of Technology (MIT). Failing to act decisively to ensure a safe learning environment for all students would be a grave dereliction of your responsibilities as President of MIT and Chair of the MIT Corporation.
This Congress will not stand idly by and allow an environment hostile to Jewish students to persist. The House believes that your institution is in violation of Title VI of the Civil Rights Act, and the inability or
unwillingness to rectify this violation through action requires accountability.
Postsecondary education is a unique opportunity for students to learn and have their ideas and beliefs challenged. However, universities receiving hundreds of millions of federal funds annually have denied
students that opportunity and have been hijacked to become venues for the promotion of terrorism, antisemitic harassment and intimidation, unlawful encampments, and in some cases, assaults and riots.
The House of Representatives will not countenance the use of federal funds to indoctrinate students into hateful, antisemitic, anti-American supporters of terrorism. Investigations into campus antisemitism by the Committee on Education and the Workforce and the Committee on Ways and Means have been expanded into a Congress-wide probe across all relevant jurisdictions to address this national crisis. The undersigned Committees will conduct oversight into the use of federal funds at MIT and its learning environment under authorities granted to each Committee.
• The Committee on Education and the Workforce has been investigating your institution since December 7, 2023. The Committee has broad jurisdiction over postsecondary education, including its compliance with Title VI of the Civil Rights Act, campus safety concerns over disruptions to the learning environment, and the awarding of federal student aid under the Higher Education Act.
• The Committee on Oversight and Accountability is investigating the sources of funding and other support flowing to groups espousing pro-Hamas propaganda and engaged in antisemitic harassment and intimidation of students. The Committee on Oversight and Accountability is the principal oversight committee of the US House of Representatives and has broad authority to investigate “any matter” at “any time” under House Rule X.
• The Committee on Ways and Means has been investigating several universities since November 15, 2023, when the Committee held a hearing entitled From Ivory Towers to Dark Corners: Investigating the Nexus Between Antisemitism, Tax-Exempt Universities, and Terror Financing. The Committee followed the hearing with letters to those institutions on January 10, 202
Macroeconomics- Movie Location
This will be used as part of your Personal Professional Portfolio once graded.
Objective:
Prepare a presentation or a paper using research, basic comparative analysis, data organization and application of economic information. You will make an informed assessment of an economic climate outside of the United States to accomplish an entertainment industry objective.
Unit 8 - Information and Communication Technology (Paper I).pdfThiyagu K
This slides describes the basic concepts of ICT, basics of Email, Emerging Technology and Digital Initiatives in Education. This presentations aligns with the UGC Paper I syllabus.
Embracing GenAI - A Strategic ImperativePeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
2. .
Outline
Introduction: Why 2UED is attractive
Survey of Positively Curved Geometries
A UED model with Bulk fermions
Localizing fermions
Conclusion: A negative future ?
Nicolas Deutschmann Curved Extra-Dimensions 2/25
...
2/25
5. .
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
Nicolas Deutschmann Curved Extra-Dimensions 5/25
...
5/25
6. .
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
Nicolas Deutschmann Curved Extra-Dimensions 5/25
...
5/25
7. .
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
Nicolas Deutschmann Curved Extra-Dimensions 5/25
...
5/25
8. .
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
• Dark Matter: often a
by-product of other
models with additional
ad hoc parity (R-parity,
KK-parity...)
Nicolas Deutschmann Curved Extra-Dimensions 5/25
...
5/25
9. .
Ad hoc parities
Many theoretically satisfying solutions to the short-comings of
the Standard Model
• Hierarchy: SuSy, RS,
Little Higgs
• Neutrinos: See-Saw
• Dark Matter: often a
by-product of other
models with additional
ad hoc parity (R-parity,
KK-parity...)
Nicolas Deutschmann Curved Extra-Dimensions 5/25
...
5/25
10. .
A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
Nicolas Deutschmann Curved Extra-Dimensions 6/25
...
6/25
11. .
A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
Nicolas Deutschmann Curved Extra-Dimensions 6/25
...
6/25
12. .
A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
• Isometries of Xn: Noether theorem imposes selection rules for
decays
Nicolas Deutschmann Curved Extra-Dimensions 6/25
...
6/25
13. .
A potential solution in the UED frame work
Universal Extra-Dimensions: all fields propagate in the bulk
• (4 + n)D space: M4 × Xn a compact space
• The eigenmodes of all fields in Xn create a KK-tower.
• Isometries of Xn: Noether theorem imposes selection rules for
decays
A stable excitation of a neutral SM field could be Dark Matter!
Nicolas Deutschmann Curved Extra-Dimensions 6/25
...
6/25
14. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
15. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
16. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
17. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
18. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
19. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
20. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
21. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
Exactly one flat geometry
(Cacciapaglia et al.)
With greater dimensions comes greater freedom
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
22. .
Why go to curved (n ≥ 2) UED ?
Two limiting factors: Isometries and fermions
1UED
Odd dimensions: no chiral
fermions
Classical trick on S1
/Z2
for a chiral zero-mode
(unique)
No symmetry
2UED
Chiral fermions, but
constructed from both
left- and right-handed
Weyls
Similar tricks for some
R2
/G
Exactly one flat geometry
(Cacciapaglia et al.)
With greater dimensions comes greater freedom
No systematic survey of curved spaces
Nicolas Deutschmann Curved Extra-Dimensions 7/25
...
7/25
23. .
Survey of Positively Curved
Geometries
Nicolas Deutschmann Curved Extra-Dimensions 8/25
...
8/25
24. .
Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
Nicolas Deutschmann Curved Extra-Dimensions 9/25
...
9/25
25. .
Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
First question: Which of these have non-trivial isometries ?
Nicolas Deutschmann Curved Extra-Dimensions 9/25
...
9/25
26. .
Positively curved geometries
.
Uniformization theorem..
.
All positively curved 2D surfaces can be described as S2
/G with
G a discrete subgroup of O(3)
First question: Which of these have non-trivial isometries ?
Fundamental relation:
S ∈ Isom(S2
/G) ⇐⇒ ∀g ∈ G, ∃h ∈ G|S(g(x)) = h(S(x))
Nicolas Deutschmann Curved Extra-Dimensions 9/25
...
9/25
28. .
Orbifolds with symmetries
(a) S2
/Cn (b) S2
/Cnh (c) S2
/Sn (d) S2
/Dn
Next question: Which of this can embed 4D chiral fermions ?
Nicolas Deutschmann Curved Extra-Dimensions 10/25
...
10/25
29. .
Orbifolds with symmetries
(a) S2
/Cn (b) S2
/Cnh (c) S2
/Sn (d) S2
/Dn
Next question: Which of this can embed 4D chiral fermions ?
Nicolas Deutschmann Curved Extra-Dimensions 10/25
...
10/25
30. .
A UED model with Bulk
fermions
Nicolas Deutschmann Curved Extra-Dimensions 11/25
...
11/25
31. .
A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Nicolas Deutschmann Curved Extra-Dimensions 12/25
...
12/25
32. .
A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
Nicolas Deutschmann Curved Extra-Dimensions 12/25
...
12/25
33. .
A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
The connection term in the two Weyl spinors of a chiral 6D
spinors become different:
χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ
Nicolas Deutschmann Curved Extra-Dimensions 12/25
...
12/25
34. .
A gauge field to kill the connection
Method from Randjbar-Daemi, Salam and Strathdee
Add an extra U(1) gauge field X
The connection term in the two Weyl spinors of a chiral 6D
spinors become different:
χ = ∂χ + (X + Ω)η η = ∂η + (X − Ω)χ
If X cancels ±Ω one of the chiralities has a zero-mode.
Nicolas Deutschmann Curved Extra-Dimensions 12/25
...
12/25
35. .
Tentative Model
Start by writing the Standard Model Lagrangian in 6D
L = LSM
Nicolas Deutschmann Curved Extra-Dimensions 13/25
...
13/25
36. .
Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
Nicolas Deutschmann Curved Extra-Dimensions 13/25
...
13/25
37. .
Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
Nicolas Deutschmann Curved Extra-Dimensions 13/25
...
13/25
38. .
Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field
L = LSM −
1
4
XµνXµν
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
How to hide this new gauge boson ?
Nicolas Deutschmann Curved Extra-Dimensions 13/25
...
13/25
39. .
Tentative Model
Start by writing the Standard Model Lagrangian in 6D with the
new gauge field and an additional Higgs field :
L = LSM −
1
4
XµνXµν
+ |DM H|2
+ µ2
|H|2
−
λ
2
|H|4
With ⟨X⟩ a magnetic monopole, fixed by GR:
⟨X⟩ =
n
2g
cos θdϕ =
√
2R
κ
cos θdϕ
How to hide this new gauge boson ?
Nicolas Deutschmann Curved Extra-Dimensions 13/25
...
13/25
40. .
Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent :
Nicolas Deutschmann Curved Extra-Dimensions 14/25
...
14/25
41. .
Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
Nicolas Deutschmann Curved Extra-Dimensions 14/25
...
14/25
42. .
Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
.
Method..
.
Minimization using
Fourier coefficients
Nicolas Deutschmann Curved Extra-Dimensions 14/25
...
14/25
43. .
Higgs Mechanism in a Monopole Background
Need to find the minimum
|DM H|2
− µ2
|H|2
+
λ
2
|H|4
A priori θ-dependent : Numerical Solution
.
Method..
.
Minimization using
Fourier coefficients
1 2 3 4 5
0.001
0.01
0.1
1
1 2 3 4 5
Mode
Αi
Nicolas Deutschmann Curved Extra-Dimensions 14/25
...
14/25
44. .
Effects of the symmetry breaking
• Higgs:
Nicolas Deutschmann Curved Extra-Dimensions 15/25
...
15/25
45. .
Effects of the symmetry breaking
• Higgs: O(1/R)
Nicolas Deutschmann Curved Extra-Dimensions 15/25
...
15/25
46. .
Effects of the symmetry breaking
• Higgs: O(1/R)
• X: g/R ∼ 10 keV
Nicolas Deutschmann Curved Extra-Dimensions 15/25
...
15/25
47. .
Effects of the symmetry breaking
• Higgs: O(1/R)
• X: g/R ∼ 10 keV
Too weak coupling for collider physics.
Compatible with short-range gravity tests
Nicolas Deutschmann Curved Extra-Dimensions 15/25
...
15/25
49. .
Spectrum of the model
SM Gauge scalar X vector Extra Higgs
0
1
2
3
4
5
6
Nicolas Deutschmann Curved Extra-Dimensions 16/25
...
16/25
50. .
Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
Nicolas Deutschmann Curved Extra-Dimensions 17/25
...
17/25
51. .
Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
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52. .
Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
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53. .
Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Tier-2 Excitations..
.
• As for Tier-1: Gluon
• If Isom(S2/G) = Z2: Single production
• Need less
√
s
• Striking jj resonance easier to look for
• Sets a limit around 1.5 − 2 TeV
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
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54. .
Some Experimental Remarks
.
X boson properties
..
.
• Interacts too weakly for colliders
• Can decay into neutrinos
(Γ ≃ 10−11 eV)
• Not a good DM candidate
.
Tier-2 Excitations..
.
• As for Tier-1: Gluon
• If Isom(S2/G) = Z2: Single production
• Need less
√
s
• Striking jj resonance easier to look for
• Sets a limit around 1.5 − 2 TeV
• Constraints can be escaped if S2/G has
a continuous symmetry
.
Extra-Higgs
..
.
No direct SM interaction so not expected at
colliders
Decay mostly into X pairs
.
Tier-1 Excitations..
.
• Need to be pair-produced
• Gluon most likely (massless zero-mode &
QCD)
• Signature: jj + ̸ET
• Loop calculation needed to raise
degeneracy with γ
• Open question: prompt decay to LKK ?
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55. .
Summing up the model
Spherical Extra-Dimensions are hard to construct.
• Chiral fermions do not come easily
• Need to add two extra-fields: X and H′
• Unsatisfying because
◦ X and H′ are rather untestable
◦ They are ugly
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57. .
Branes, fat branes and all that
Bottom-up
All but one symmetric
orbifolds have singular
points
• QFT argument:
localized counter-terms
• GR argument: branes
Top-Bottom ∃ explicit
examples of localization:
• RS (not relevant)
• Georgi mechanism on
S1
/Z2
Nice for later if the model
is phenomenologically
relevant.
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58. .
What the model looks like
• Specific orbifold
choice: S2
/S4
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59. .
What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
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60. .
What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
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61. .
What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
• first tier: unstable
scalars (loop-level)
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62. .
What the model looks like
l=0
l=2
l=3
m=0m=-2 m=2
l=1
• Specific orbifold
choice: S2
/S4
• 6D QCD+EW
• 4D Standard model
fermion content with
gauge couplings to the
4D gauge vectors
• first tier: unstable
scalars (loop-level)
• second tier: unstable
vectors, stable scalars
(DM)
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63. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level:
• Tier-2 excitations provide resonances:
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
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64. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances:
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
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65. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon:
• Direct detection:
• Relic density:
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66. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection:
• Relic density:
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67. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection: hard because loop-suppressed
• Relic density:
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68. .
Phenomenology
Two competing constraints: LHC v.s. Dark Matter
.
LHC constraints..
.
• Tier-1 excitations couple at loop level: sub-dominant a priori
• Tier-2 excitations provide resonances: R ≥ 1.5 TeV
.
Dark matter..
.
Likely DM candidate: scalar Tier-2 photon: WIMPZILLA!
• Direct detection: hard because loop-suppressed
• Relic density: needs loop calculations
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70. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
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71. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
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72. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
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73. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
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74. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
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75. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
• Topological constraints (genus↔ V/Rn
) make the curvature
radius the only thing to stabilize
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76. .
A Brighter Horizon: Hyperbolic Extra-Dimensions
• Fermions behave much more nicely: there is a massless mode
• Much more freedom: arbitrary high volumes for a given
curvature radius
• Mass gap protected by curvature radius
• Can pull down Mpl while keeping MKK high enough
• Many features attractive for cosmology (flatness, uniformity,
inflation, ...)
• Topological constraints (genus↔ V/Rn
) make the curvature
radius the only thing to stabilize
• Quantum corrections could play a significant role as Mpl goes
down
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77. .
Thank you for your attention
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