Large Mass Hierarchy from a Small Extra Dimension
|
|
- Darren Erick Harper
- 5 years ago
- Views:
Transcription
1 Large Mass Hierarchy from a Small Extra Dimension Sridip Pal (09MS002) DPS PH4204 April 4,2013 Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
2 Outline 1 Introduction What is Hierarchy Problem 2 Kaluza Klein Action 3 ADD Compactification 4 Solution to Hierarchy in ADD Model Hierarchy in Disguise 5 Randall-Sundrum Model 6 Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
3 Hierarchy Problem Introduction What is Hierarchy Problem The gravity is weak compared to other fundamental forces. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
4 Hierarchy Problem Introduction What is Hierarchy Problem The gravity is weak compared to other fundamental forces. The gravitational coupling constant G 4d = M 2 Pl = GeV 2. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
5 Hierarchy Problem Introduction What is Hierarchy Problem The gravity is weak compared to other fundamental forces. The gravitational coupling constant G 4d = M 2 Pl = GeV 2. It is weak in the sense G 4d m 2 p = << 1. and G 4d ν 2 = << 1 Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
6 Introduction What is Hierarchy Problem Hierarchy Problem The gravity is weak compared to other fundamental forces. The gravitational coupling constant G 4d = M 2 Pl = GeV 2. It is weak in the sense G 4d m 2 p = << 1. and G 4d ν 2 = << 1 Gravity becomes dominant when elementary particle becomes as heavy as GeV. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
7 Introduction What is Hierarchy Problem Hierarchy Problem The gravity is weak compared to other fundamental forces. The gravitational coupling constant G 4d = M 2 Pl = GeV 2. It is weak in the sense G 4d m 2 p = << 1. and G 4d ν 2 = << 1 Gravity becomes dominant when elementary particle becomes as heavy as GeV. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
8 Hierarchy Problem Introduction What is Hierarchy Problem Standard Model does not incorporate gravity and we can safely ignore it as it is a force. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
9 Introduction What is Hierarchy Problem Hierarchy Problem Standard Model does not incorporate gravity and we can safely ignore it as it is a force. But we cant expect Standard Model to be valid at energy scale GeV where Gravity becomes strong. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
10 Introduction What is Hierarchy Problem Hierarchy Problem Standard Model does not incorporate gravity and we can safely ignore it as it is a force. But we cant expect Standard Model to be valid at energy scale GeV where Gravity becomes strong. So Standard Model has a natural cut off at GeV. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
11 Introduction What is Hierarchy Problem Hierarchy Problem Standard Model does not incorporate gravity and we can safely ignore it as it is a force. But we cant expect Standard Model to be valid at energy scale GeV where Gravity becomes strong. So Standard Model has a natural cut off at GeV. Loop correction renders Higgs mass as high as GeV because the divergence is quadratic. m 2 = m ( 10 19) 2 (1) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
12 Introduction What is Hierarchy Problem Hierarchy Problem Standard Model does not incorporate gravity and we can safely ignore it as it is a force. But we cant expect Standard Model to be valid at energy scale GeV where Gravity becomes strong. So Standard Model has a natural cut off at GeV. Loop correction renders Higgs mass as high as GeV because the divergence is quadratic. m 2 = m ( 10 19) 2 If we want to have m = 125GeV,the bare mass m 0 has to be very large, hence m/m 0 has to be very precise which is unnatural and termed Fine Tuning Problem. (1) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
13 Introduction What is Hierarchy Problem Hierarchy Problem Hierarchy problem is about Why weak scale (ν) is so small compared to M Pl = GeV. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
14 Introduction What is Hierarchy Problem Hierarchy Problem Hierarchy problem is about Why weak scale (ν) is so small compared to M Pl = GeV. In other words why gravity is so weak. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
15 Introduction What is Hierarchy Problem Hierarchy Problem Hierarchy problem is about Why weak scale (ν) is so small compared to M Pl = GeV. In other words why gravity is so weak. Is there any solution to fine tunning problem? Can we aviod such fine tuning of parameter like Higgs mass.? Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
16 Kaluza Klein Action Action in General Relativity and KK Action S GR = 1 16πG 4D d 4 x gr (2) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
17 Kaluza Klein Action Action in General Relativity and KK Action S GR = 1 16πG 4D d 4 x gr (2) Kaluza Klein action is simple generalisation of above action 1 S KK = d 5 x g 16πG R (3) 5D Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
18 Kaluza Klein Action Action in General Relativity and KK Action S GR = 1 16πG 4D d 4 x gr (2) Kaluza Klein action is simple generalisation of above action 1 S KK = d 5 x g 16πG R (3) 5D g = kg (4) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
19 Kaluza Klein Action Action in General Relativity and KK Action S GR = 1 16πG 4D d 4 x gr (2) Kaluza Klein action is simple generalisation of above action 1 S KK = d 5 x g 16πG R (3) 5D g = kg (4) R = R 1 4 F αβf αβ (5) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
20 Compactification Kaluza Klein Action S KK = k 16πG 5D dx 5 d 4 x g [R k4 ] F αβf αβ (6) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
21 Compactification Kaluza Klein Action S KK = k 16πG 5D dx 5 d 4 x g [R k4 ] F αβf αβ (6) Figure: Compactified Extra Dimension Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
22 Kaluza Klein Action Kaluza Klein Action continued.. Assuming cylindrical compactification of extra dimension with radius a we get S KK = 2πa k d 4 x g [R k4 ] 16πG F αβf αβ (7) 5D Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
23 Kaluza Klein Action Kaluza Klein Action continued.. Assuming cylindrical compactification of extra dimension with radius a we get S KK = 2πa k d 4 x g [R k4 ] 16πG F αβf αβ (7) 5D 1 S GR = d 4 x gr (8) 16πG 4D Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
24 Kaluza Klein Action Kaluza Klein Action continued.. Assuming cylindrical compactification of extra dimension with radius a we get S KK = 2πa k d 4 x g [R k4 ] 16πG F αβf αβ (7) 5D 1 S GR = d 4 x gr (8) 16πG 4D G 4D = G 5D 2πa k (9) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
25 4+n Dimension ADD Compactification ds 2 = g AB dx A dx B = g µν dx µ dx ν + γ ij dy i dy j (10) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
26 4+n Dimension ADD Compactification ds 2 = g AB dx A dx B = g µν dx µ dx ν + γ ij dy i dy j (10) R[ g AB ] = R[g µν ] + R[γ ij ] (11) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
27 4+n Dimension ADD Compactification ds 2 = g AB dx A dx B = g µν dx µ dx ν + γ ij dy i dy j (10) The determinant of the metric is given by R[ g AB ] = R[g µν ] + R[γ ij ] (11) g = gγ (12) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
28 ADD Compactification The action is given by 1 S = 16πG 4+n d 4+n x gr[ g AB ] (13) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
29 ADD Compactification The action is given by 1 S = 16πG 4+n d 4+n x gr[ g AB ] (13) We assume the extradimensions are compactified in a volume V n V n = d n y γ (14) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
30 ADD Compactification The action is given by 1 S = 16πG 4+n d 4+n x gr[ g AB ] (13) We assume the extradimensions are compactified in a volume V n V n = d n y γ (14) S eff = V n 16πG 4+n d 4 x g (R[g µν ] + 1Vn d n y ) γr[γ ij ] (15) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
31 ADD Compactification The action is given by 1 S = 16πG 4+n d 4+n x gr[ g AB ] (13) We assume the extradimensions are compactified in a volume V n V n = d n y γ (14) S eff = V n 16πG 4+n d 4 x g (R[g µν ] + 1Vn d n y ) γr[γ ij ] (15) V n G 4+n = 1 G 4 (16) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
32 Solution to Hierarchy in ADD Model Hieararchy Explained! where M 2 Pl = Mn+2 µ n c (17) M Pl corresponds to 4 dimensional reduced Planck scale and M represents fundamental Planck scale in higher D theory and µ c is the scale of compactification. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
33 Solution to Hierarchy in ADD Model Hieararchy Explained! M 2 Pl = Mn+2 µ n c (17) where M Pl corresponds to 4 dimensional reduced Planck scale and M represents fundamental Planck scale in higher D theory and µ c is the scale of compactification. M = 1TeV, M Pl = GeV leading to µ c = n TeV. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
34 Solution to Hierarchy in ADD Model Hieararchy Explained! M 2 Pl = Mn+2 µ n c (17) where M Pl corresponds to 4 dimensional reduced Planck scale and M represents fundamental Planck scale in higher D theory and µ c is the scale of compactification. M = 1TeV, M Pl = GeV leading to µ c = n TeV. Size of the extradimension is given by r c = 1 µ c = n cm Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
35 Solution to Hierarchy in ADD Model Hieararchy Explained! M 2 Pl = Mn+2 µ n c (17) where M Pl corresponds to 4 dimensional reduced Planck scale and M represents fundamental Planck scale in higher D theory and µ c is the scale of compactification. M = 1TeV, M Pl = GeV leading to µ c = n TeV. Size of the extradimension is given by r c = 1 µ c = n cm n=1 is simply ruled out beacuse it is too large; so this compactification model requires n 2. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
36 Solution to Hierarchy in ADD Model Hieararchy Explained! M 2 Pl = Mn+2 µ n c (17) where M Pl corresponds to 4 dimensional reduced Planck scale and M represents fundamental Planck scale in higher D theory and µ c is the scale of compactification. M = 1TeV, M Pl = GeV leading to µ c = n TeV. Size of the extradimension is given by r c = 1 µ c = n cm n=1 is simply ruled out beacuse it is too large; so this compactification model requires n 2. For n=2 we extra dimension of 1 mm size. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
37 Solution to Hierarchy in ADD Model Hierarchy in Disguise Hierarchy in Disguise This scenario does eliminate the hierarchy between weak scale ν (TeV) and Planck Scale, it introduces a new hierarchy between ν and µ c 1 V n Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
38 Solution to Hierarchy in ADD Model Hierarchy in Disguise Hierarchy in Disguise This scenario does eliminate the hierarchy between weak scale ν (TeV) and Planck Scale, it introduces a new hierarchy between ν and µ c 1 V n µ c ν = n (18) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
39 Randall-Sundrum Model Randall Sundrum Model This model is distinct from the previous in following points: There is only one extra dimension involved as opposed to n 2. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
40 Randall-Sundrum Model Randall Sundrum Model This model is distinct from the previous in following points: There is only one extra dimension involved as opposed to n 2. There is no such disguised hierarchy between weak scale and compactification scale. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
41 Randall-Sundrum Model Randall Sundrum Model This model is distinct from the previous in following points: There is only one extra dimension involved as opposed to n 2. There is no such disguised hierarchy between weak scale and compactification scale. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
42 Set Up Randall-Sundrum Model The geometry is nonfactorizable with following form ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (19) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
43 Set Up Randall-Sundrum Model The geometry is nonfactorizable with following form ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (19) The topology of the extradimension is S 1 /Z 2. The 5th coordinate is angular in nature with (x, φ) identified with (x, φ). Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
44 Randall-Sundrum Model Set Up The geometry is nonfactorizable with following form ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (19) The topology of the extradimension is S 1 /Z 2. The 5th coordinate is angular in nature with (x, φ) identified with (x, φ). The 3-branes extending in x µ direction are located at φ = 0 and φ = π. gµν vis = G µν (x µ, φ = π) (20) gµν hid = G µν (x µ, φ = 0) (21) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
45 Set up Randall-Sundrum Model Figure: Randall Sundrum Model Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
46 The Classical Action Randall-Sundrum Model S = S gravity + S vis + S hid (22) where S gravity = d 4 x π π dφ G[ Λ + 2M 3 R] (23) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
47 The Classical Action Randall-Sundrum Model S = S gravity + S vis + S hid (22) where S gravity = d 4 x S vis = π π dφ G[ Λ + 2M 3 R] (23) d 4 x g vis [L vis V vis ] (24) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
48 The Classical Action Randall-Sundrum Model S = S gravity + S vis + S hid (22) where π S gravity = d 4 x dφ G[ Λ + 2M 3 R] (23) π S vis = d 4 x g vis [L vis V vis ] (24) S hid = d 4 x g hid [L hid V hid ] (25) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
49 The Classical Action Randall-Sundrum Model S = S gravity + S vis + S hid (22) where π S gravity = d 4 x dφ G[ Λ + 2M 3 R] (23) π S vis = d 4 x g vis [L vis V vis ] (24) S hid = d 4 x g hid [L hid V hid ] (25) where V vis and V hid is vacuum energy of the branes which act as a gravitational source even in absence of matter on brane. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
50 Randall-Sundrum Model Solution for the Bulk Metric ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (26) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
51 Randall-Sundrum Model Solution for the Bulk Metric ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (26) where ds 2 = e 2krc φ η µν dx µ dx ν + r 2 c dφ 2 (27) k = Λ 24M 3 (28) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
52 Randall-Sundrum Model Solution for the Bulk Metric ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (26) ds 2 = e 2krc φ η µν dx µ dx ν + r 2 c dφ 2 (27) where Λ k = 24M 3 (28) To satisty the Einstein s equation, we must have V vis = V hid = 24M 3 (29) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
53 Randall-Sundrum Model Solution for the Bulk Metric ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (26) ds 2 = e 2krc φ η µν dx µ dx ν + r 2 c dφ 2 (27) where Λ k = 24M 3 (28) To satisty the Einstein s equation, we must have V vis = V hid = 24M 3 (29) Demanding a metric with a warp factor forces the existence of branes at φ = 0 and φ = π with vacuum energy given by above. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
54 Randall-Sundrum Model Solution for the Bulk Metric ds 2 = e 2σ(φ) η µν dx µ dx ν + r 2 c dφ 2 (26) ds 2 = e 2krc φ η µν dx µ dx ν + r 2 c dφ 2 (27) where Λ k = 24M 3 (28) To satisty the Einstein s equation, we must have V vis = V hid = 24M 3 (29) Demanding a metric with a warp factor forces the existence of branes at φ = 0 and φ = π with vacuum energy given by above. The bulk has negative Λ-hence the bulk is a slice of AdS 5 geometry. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
55 Weak Scale from Planck Scale Relation between M and M Pl We perturb the background metric so that ds 2 = e 2krc φ [η µν + h µν ]dx µ dx ν + r 2 c dφ 2 (30) where h µν is tensor fluctuations about Minkowski spacetime. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
56 Weak Scale from Planck Scale Relation between M and M Pl We perturb the background metric so that ds 2 = e 2krc φ [η µν + h µν ]dx µ dx ν + r 2 c dφ 2 (30) where h µν is tensor fluctuations about Minkowski spacetime. The 4dimensional effective theory follows by substituting the above in S gravity = d 4 x π π dφ G[ Λ + 2M 3 R] Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
57 Contd.. Weak Scale from Planck Scale S eff d 4 x π π dφ2m 3 r c e 2krc φ ḡ R (31) where R denotes the 4 dimensional Ricci scalar made out of ḡ µν. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
58 Contd.. Weak Scale from Planck Scale S eff d 4 x π π dφ2m 3 r c e 2krc φ ḡ R (31) where R denotes the 4 dimensional Ricci scalar made out of ḡ µν. M 2 Pl = M 3 r c π π dφe 2krc φ = M3 k [ 1 e 2krc φ ] (32) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
59 Contd.. Weak Scale from Planck Scale S eff d 4 x π π dφ2m 3 r c e 2krc φ ḡ R (31) where R denotes the 4 dimensional Ricci scalar made out of ḡ µν. M 2 Pl = M 3 r c π π dφe 2krc φ = M3 k [ 1 e 2krc φ ] (32) M Pl depends weakly on r c in the large kr c limit. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
60 Contd.. Weak Scale from Planck Scale S eff d 4 x π π dφ2m 3 r c e 2krc φ ḡ R (31) where R denotes the 4 dimensional Ricci scalar made out of ḡ µν. M 2 Pl = M 3 r c π π dφe 2krc φ = M3 k [ 1 e 2krc φ ] (32) M Pl depends weakly on r c in the large kr c limit. But the exponential hierarchy plays a crucial role in determining visible sector masses. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
61 Scaling of Mass Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy S vis d 4 x g vis [g µν vis D µh D ν H λ( H 2 ν 2 0) 2 ] (33) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
62 Scaling of Mass Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy S vis d 4 x g vis [g µν vis D µh D ν H λ( H 2 ν 2 0) 2 ] (33) Now substitute g µν vis = e2krcπ ḡ µν (34) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
63 Scaling of Mass Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy S vis d 4 x g vis [g µν vis D µh D ν H λ( H 2 ν 2 0) 2 ] (33) Now substitute g µν vis = e2krcπ ḡ µν (34) So we have S vis d 4 x ḡe 4krcπ [ḡ µν e 2krcπ D µ H D ν H λ( H 2 ν 2 0) 2 ] (35) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
64 Weak Scale from Planck Scale Exponential Hierarchy Visible Sector Mass-Exponential Hierarchy We rescale H e krcπ H (36) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
65 Weak Scale from Planck Scale Exponential Hierarchy Visible Sector Mass-Exponential Hierarchy We rescale we obtain S vis H e krcπ H (36) d 4 x ḡ[ḡ µν D µ H D ν H λ( H 2 e 2krcπ ν 2 0) 2 ] (37) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
66 Weak Scale from Planck Scale Exponential Hierarchy Visible Sector Mass-Exponential Hierarchy We rescale we obtain S vis H e krcπ H (36) d 4 x ḡ[ḡ µν D µ H D ν H λ( H 2 e 2krcπ ν 2 0) 2 ] (37) ν = e krcπ ν 0 (38) Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
67 Scaling of Mass Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy m = e krcπ m 0 (39) If e krcπ is of the order of the mechanism produces TeV physical mass scale from Plank scale (10 19 GeV ). Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
68 Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy Scaling of Mass m = e krcπ m 0 (39) If e krcπ is of the order of the mechanism produces TeV physical mass scale from Plank scale (10 19 GeV ). Because the warping factor is exponential the model does not require very large hierarchies among fundamental parameters ν 0,k,M and µ c = 1 r c ; with kr c 10. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
69 Weak Scale from Planck Scale Generation of Exponential Hierarchy Visible Sector Mass-Exponential Hierarchy Figure: Generation of Exponential Hierarchy Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
70 Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy References Kaluza Klein Theory, William.O.Straub,PhD, Pasadena, California ( Kaluza Klein Theories, David Bailin and Alex Love, Rep. Prog. Phys. 50, 1087 (1987) A First Course in String Theory, Barton Zwiebach, Second Edition Large Mass Hierarchy from a Small Extra Dimension, L.Randall and R.Sundrum, Phys. Rev. Lett. 83, 3370 (1999). The Aim of the Talk is to present the above paper by Randall, Sundrum. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
71 Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy Acknowledgement The speaker acknowdeges a debt of gratitude to Dr.G.M.Hossain, Dept. of Physical Science, IISER Kolkata Prof.N.Banarjee, Dept. of Physical Science, IISER Kolkata Prof.S.Sengupta, Dept. of Theoretical Physics, IACS for their valuable time and guidance. Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
72 Weak Scale from Planck Scale Visible Sector Mass-Exponential Hierarchy THANK YOU Sridip Pal (09MS002) DPS PH4204 () Large Mass Hierarchy from a Small Extra Dimension April 4, / 26
Thick Brane World. Seyen Kouwn Korea Astronomy and Space Science Institute Korea
Thick Brane World Seyen Kouwn Korea Astronomy and Space Science Institute Korea Introduction - Multidimensional theory 1 Why are the physically observed dimensions of our Universe = 3 + 1 (space + time)?
More informationSTABILIZATION OF MODULUS IN RANDALL SUNDRUM MODEL I BY BULK SCALAR FIELDS
Modern Physics Letters A Vol. 28, No. 11 (2013) 1350044 (6 pages) c World Scientific Publishing Company DOI: 10.1142/S0217732313500442 STABILIZATION OF MODULUS IN RANDALL SUNDRUM MODEL I BY BULK SCALAR
More informationBrane world scenarios
PRAMANA cfl Indian Academy of Sciences Vol. 60, No. 2 journal of February 2003 physics pp. 183 188 Brane world scenarios DILEEP P JATKAR Harish-Chandra Research Institute, Chhatnag Road, Jhusi, Allahabad
More information...and the extradimensions quest
A brief introduction to the Randall-Sundrum Models...and the extradimensions quest Bruno BERTRAND Center for particle physics and phenomenology (CP3) CP3 Seminar : Randall-Sundrum models - Bruno BERTRAND
More informationLarge Extra Dimensions and the Hierarchy Problem
Large Extra Dimensions and the Hierarchy Problem The Hierarchy Problem - At Planck energies (M P L 10 19 GeV ) all four forces have the same strength. -At the Electroweak scale (M EW 1T ev ) the four forces
More informationSearching for Extra Space Dimensions at the LHC. M.A.Parker Cavendish Laboratory Cambridge
Searching for Extra Space Dimensions at the LHC M.A.Parker Cavendish Laboratory Cambridge I shall use ATLAS to illustrate LHC physics, because it is the experiment I know best. Both general purpose detectors
More informationWarped Models in String Theory
Warped Models in String Theory SISSA/ISAS Trieste (Italy) Rutgers 14 November 2006 (Work in collaboration with B.S.Acharya and F.Benini) Appearing soon Introduction 5D Models 5D warped models in a slice
More informationScalar field dark matter and the Higgs field
Scalar field dark matter and the Higgs field Catarina M. Cosme in collaboration with João Rosa and Orfeu Bertolami Phys. Lett., B759:1-8, 2016 COSMO-17, Paris Diderot University, 29 August 2017 Outline
More informationInter-brane distance stabilization by bulk Higgs field in RS model
EPJ Web of Conferences 58, 0500 07 QFTHEP 07 DOI: 0.05/epjconf/07580500 Inter-brane distance stabilization by bulk Higgs field in RS model Vadim Egorov,, and Igor Volobuev, Skobeltsyn Institute of Nuclear
More informationD. f(r) gravity. φ = 1 + f R (R). (48)
5 D. f(r) gravity f(r) gravity is the first modified gravity model proposed as an alternative explanation for the accelerated expansion of the Universe [9]. We write the gravitational action as S = d 4
More informationS = 2 decay in Warped Extra Dimensions
S = 2 decay in Warped Extra Dimensions Faisal Munir IHEP, Beijing Supervisor: Cai-Dian Lü HFCPV CCNU, Wuhan October 28, 2017 based on: Chin. Phys. C41 (2017) 053106 [arxiv:1607.07713] F. Munir (IHEP) New
More informationBEYOND THE SM (II) Kaustubh Agashe (University of Maryland)
BEYOND THE SM (II) Kaustubh Agashe (University of Maryland) ierarchy problems (from lecture 1) Planck-weak hierarchy problem Flavor (hierarchy) puzzle...extra dimensions can address both... Extra dimensions:
More informationThe Randall-Sundrum model
The Randall-Sundrum model Aleksandr Chatrchyan & Björn Jüliger After a brief non-technical introduction to the Hierarchy problem, we first discuss the old five-dimensional Kaluza-Klein model, its tower
More informationAccidental SUSY at the LHC
Accidental SUSY at the LHC Tony Gherghetta (University of Melbourne) PACIFIC 2011, Moorea, French Polynesia, September 12, 2011 with Benedict von Harling and Nick Setzer [arxiv:1104.3171] 1 What is the
More informationDoes a Randall-Sundrum scenario create the illusion of a torsion-free universe?
hep-th/0204242 Does a Randall-Sundrum scenario create the illusion of a torsion-free universe? Biswarup Mukhopadhyaya 1, Somasri Sen 2 Harish-Chandra Research Institute, Chhatnag Road, Jhusi, Allahabad
More informationLife with More Than 4: Extra Dimensions
Life with More Than 4: Extra Dimensions Andrew Larkoski 4/15/09 Andrew Larkoski SASS 5 Outline A Simple Example: The 2D Infinite Square Well Describing Arbitrary Dimensional Spacetime Motivations for Extra
More informationGeneral Warped Solution in 6d Supergravity. Christoph Lüdeling
General Warped Solution in 6d Supergravity Christoph Lüdeling DESY Hamburg DPG-Frühjahrstagung Teilchenphysik H. M. Lee, CL, JHEP 01(2006) 062 [arxiv:hep-th/0510026] C. Lüdeling (DESY Hamburg) Warped 6d
More informationBRANE COSMOLOGY and Randall-Sundrum model
BRANE COSMOLOGY and Randall-Sundrum model M. J. Guzmán June 16, 2009 Standard Model of Cosmology CMB and large-scale structure observations provide us a high-precision estimation of the cosmological parameters:
More informationIntroduction to the Beyond the Standard Model session
Introduction to the Beyond the Standard Model session JRJC 2015 Nov. 19th 2015 Samuel Calvet Outline Why do we need Beyond the Standard Model (BSM) theories? BSM theories on the market : their predictions/particles
More informationELECTROWEAK BREAKING IN EXTRA DIMENSIONS MINI REVIEW. Gero von Gersdorff (École Polytechnique) Moriond Electroweak Session, La Thuile, March 2011
ELECTROWEAK BREAKING IN EXTRA DIMENSIONS MINI REVIEW Gero von Gersdorff (École Polytechnique) Moriond Electroweak Session, La Thuile, March 2011 OUTLINE How can Extra Dimensions explain the electroweak
More informationIntroduction to the Beyond the Standard Model session
Introduction to the Beyond the Standard Model session JJC 2014 Dec. 11th 2014 Samuel Calvet Outline Why do we need Beyond the Standard Model (BSM) theories? BSM theories on the market : their predictions/particles
More informationTHE GEOMETRY OF THE TORUS UNIVERSE
International Journal of Modern Physics D Vol. 16, No. 4 (2007) 681 686 c World Scientific Publishing Company THE GEOMETRY OF THE TORUS UNIVERSE R. MURDZEK Physics Department, Al. I. Cuza University, Iassy,
More informationarxiv:gr-qc/ v1 4 Jun 2003
Wormhole solutions in the Randall-Sundrum scenario M. La Camera Department of Physics and INFN - University of Genoa Via Dodecaneso 33, 16146 Genova, Italy Abstract In the simplest form of the Randall-Sundrum
More informationGravity in the Braneworld and
Gravity in the Braneworld and the AdS/CFT Correspondence Takahiro TANAKA Department of Physics, Kyoto University, Kyoto 606-8502, Japan October 18, 2004 Abstract We discuss gravitational interaction realized
More informationIntroduction to (Large) Extra Dimensions
SLAC Dark Matter & Exotic Physics WG p. 1/39 Introduction to (Large) Extra Dimensions A. Lionetto Department of Physics & INFN Roma Tor Vergata SLAC Dark Matter & Exotic Physics WG p. 2/39 Outline Introduction
More informationarxiv:hep-ph/ v2 30 Aug 2002
LPNHE-00-05 arxiv:hep-ph/007166v 30 Aug 00 Search for Extra Space-Dimensions at the LHC B. Laforge Laboratoire de Physique Nucléaire et de Hautes Energies CNRS-INP3 et Universités Paris VI & VII France
More informationScalar fields and higher-derivative gravity in brane worlds
Scalar fields and higher-derivative gravity in brane worlds Dissertation of the faculty of physics of the Ludwig-Maximilians-Universität München submitted by Sebastian Pichler from Trostberg Munich, November
More information1. Introduction. [Arkani-Hamed, Dimopoulos, Dvali]
2014 Ï Ò (í «) Ò Ò Ù Åǽ À 20145 7 Content 1. Introduction and Motivation 2. f(r)-brane model and solutions 3. Localization of gravity on f(r)-brane 4. Gravity resonances on f(r)-brane 5. Corrections to
More informationSearching for Extra Space Dimensions at the LHC. M.A.Parker Cavendish Laboratory Cambridge
Searching for Extra Space Dimensions at the LHC M.A.Parker Cavendish Laboratory Cambridge The Large Hadron Collider Under construction in Geneva, startup in 2007. 14 TeV pp collider, L=1034cm-2 s-1. σ
More informationarxiv:hep-th/ v1 8 Jun 1999
hep-th/9906064 MIT-CTP-2874 PUPT-1867 BUHEP-99-13 An Alternative to Compactification arxiv:hep-th/9906064v1 8 Jun 1999 Lisa Randall Joseph Henry Laboratories, Princeton University, Princeton, NJ 08543,
More informationBraneworlds: gravity & cosmology. David Langlois APC & IAP, Paris
Braneworlds: gravity & cosmology David Langlois APC & IAP, Paris Outline Introduction Extra dimensions and gravity Large (flat) extra dimensions Warped extra dimensions Homogeneous brane cosmology Brane
More informationbrane world cosmology An introduction to Andreas Müller Theory group LSW Advanced seminar LSW Heidelberg 03/03/2004
An introduction to brane world cosmology Andreas Müller Theory group LSW http://www.lsw.uni-heidelberg.de/users/amueller Advanced seminar LSW Heidelberg 03/03/2004 Overview principles bulk and brane extradimensions
More informationLecturer: Bengt E W Nilsson
9 3 19 Lecturer: Bengt E W Nilsson Last time: Relativistic physics in any dimension. Light-cone coordinates, light-cone stuff. Extra dimensions compact extra dimensions (here we talked about fundamental
More informationOn the stabilization of modulus in Randall Sundrum model by R 2 interaction
PRAMANA c Indian Academy of Sciences Vol. 86, No. 3 journal of March 206 physics pp. 537 543 On the stabilization of modulus in Randall Sundrum model by R 2 interaction A TOFIGHI Department of Nuclear
More informationTheories with Compact Extra Dimensions
Instituto de Física USP PASI 2012 UBA Theories with Compact Extra dimensions Part II Generating Large Hierarchies with ED Theories Warped Extra Dimensions Warped Extra Dimensions One compact extra dimension.
More informationINTRODUCTION TO EXTRA DIMENSIONS
INTRODUCTION TO EXTRA DIMENSIONS MARIANO QUIROS, ICREA/IFAE MORIOND 2006 INTRODUCTION TO EXTRA DIMENSIONS p.1/36 OUTLINE Introduction Where do extra dimensions come from? Strings and Branes Experimental
More informationAre spacetime horizons higher dimensional sources of energy fields? (The black hole case).
Are spacetime horizons higher dimensional sources of energy fields? (The black hole case). Manasse R. Mbonye Michigan Center for Theoretical Physics Physics Department, University of Michigan, Ann Arbor,
More informationarxiv: v1 [hep-th] 3 Feb 2016
Noname manuscript No. (will be inserted by the editor) Thermodynamics of Asymptotically Flat Black Holes in Lovelock Background N. Abbasvandi M. J. Soleimani Shahidan Radiman W.A.T. Wan Abdullah G. Gopir
More informationString Phenomenology ???
String Phenomenology Andre Lukas Oxford, Theoretical Physics d=11 SUGRA IIB M IIA??? I E x E 8 8 SO(32) Outline A (very) basic introduction to string theory String theory and the real world? Recent work
More informationWarp Duality in Braneworlds
Warp Duality in Braneworlds Andrew B. McGowan September 14, 2007 Abstract In recent years there have emerged numerous models of spacetime that include extra dimensions. In particular there have been a
More informationThe Correct Interpretation of the Kaluza-Klein Theory
Copyright 2014 by Sylwester Kornowski All rights reserved The Correct Interpretation of the Kaluza-Klein Theory Sylwester Kornowski Abstract: Here, within the Scale-Symmetric Everlasting Theory (S-SET),
More informationDomain Wall Brane in Eddington Inspired Born-Infeld Gravity
2012cüWâfÔn»Æï? Domain Wall Brane in Eddington Inspired Born-Infeld Gravity µ4œ Ç =²ŒÆnØÔnïÄ Email: yangke09@lzu.edu.cn I# Ÿ 2012.05.10 Outline Introduction to Brane World Introduction to Eddington Inspired
More informationAharonov-Bohm Effect and Unification of Elementary Particles. Yutaka Hosotani, Osaka University Warsaw, May 2006
Aharonov-Bohm Effect and Unification of Elementary Particles Yutaka Hosotani, Osaka University Warsaw, May 26 - Part 1 - Aharonov-Bohm effect Aharonov-Bohm Effect! B)! Fµν = (E, vs empty or vacuum!= Fµν
More informationTheory and phenomenology of hidden U(1)s from string compactifications
Theory and phenomenology of hidden U(1)s from string compactifications Andreas Ringwald DESY Corfu Summer Institute Workshop on Cosmology and Strings, Sept. 6-13, 2009, Corfu, GR Theory and phenomenology
More informationBrief course of lectures at 18th APCTP Winter School on Fundamental Physics
Brief course of lectures at 18th APCTP Winter School on Fundamental Physics Pohang, January 20 -- January 28, 2014 Motivations : (1) Extra-dimensions and string theory (2) Brane-world models (3) Black
More informationSTABILIZING EXTRA DIMENSIONS
STABILIZING EXTRA DIMENSIONS Gero von Gersdorff (École Polytechnique) Warsaw, October 19th 2009 Collaboration with J.A.Cabrer and M.Quirós OUTLINE Features of Warped Extra Dimensions Stabilizing Models
More informationHolographic self-tuning of the cosmological constant
Holographic self-tuning of the cosmological constant Francesco Nitti Laboratoire APC, U. Paris Diderot IX Aegean Summer School Sifnos, 19-09-2017 work with Elias Kiritsis and Christos Charmousis, 1704.05075
More informationGravitational perturbations on branes
º ( Ò Ò ) Ò ± 2015.4.9 Content 1. Introduction and Motivation 2. Braneworld solutions in various gravities 2.1 General relativity 2.2 Scalar-tensor gravity 2.3 f(r) gravity 3. Gravitational perturbation
More informationDilaton gravity at the brane with general matter-dilaton coupling
Dilaton gravity at the brane with general matter-dilaton coupling University of Würzburg, Institute for Theoretical Physics and Astrophysics Bielefeld, 6. Kosmologietag May 5th, 2011 Outline introduction
More informationarxiv: v2 [hep-ph] 8 Mar 2018
Exploring extra dimensions through inflationary tensor modes Sang Hui Im, Hans Peter Nilles, Andreas Trautner arxiv:1707.03830v [hep-ph] 8 Mar 018 Bethe Center for Theoretical Physics and Physikalisches
More informationSolutions to gauge hierarchy problem. SS 10, Uli Haisch
Solutions to gauge hierarchy problem SS 10, Uli Haisch 1 Quantum instability of Higgs mass So far we considered only at RGE of Higgs quartic coupling (dimensionless parameter). Higgs mass has a totally
More informationq form field and Hodge duality on brane
Lanzhou University (=²ŒÆ) With C.E. Fu, H. Guo and S.L. Zhang [PRD 93 (206) 064007] 4th International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry December 29-3, 206, December 3,
More informationFLAVOUR IN WARPED EXTRA DIMENSIONS
FLAVOUR IN WARPED EXTRA DIMENSIONS G. CACCIAPAGLIA Institut de Physique Nucléaire de Lyon, Université Lyon, CNRS/IN2P3, F-69622 Villeurbanne Cedex, France Models in warped extra dimensions are very attractive
More informationBrane-World Black Holes
Brane-World Black Holes A. Chamblin, S.W. Hawking and H.S. Reall DAMTP University of Cambridge Silver Street, Cambridge CB3 9EW, United Kingdom. Preprint DAMTP-1999-133 arxiv:hep-th/990905v 1 Oct 1999
More informationClassical and Quantum Fields in Brane Worlds
Classical and Quantum Fields in Brane Worlds Alan Knapman A Thesis Submitted to the University of Newcastle Upon Tyne for the Degree of Doctor of Philosophy School of Mathematics & Statistics Newcastle
More informationBraneworld in f(r) gravity and critical gravity
Braneworld in f(r) gravity and critical gravity Yu-Xiao Liu Institute of Theoretical Physics, Lanzhou University ICTS, USTC, Hefei 2011.12.13 Content Introduction and motivation f(r) thick brane f(r) thick
More informationarxiv: v1 [physics.gen-ph] 9 May 2014
arxiv:1407.6624v1 [physics.gen-ph] 9 May 2014 Vanishing Dimensions in Four Dimensional Cosmology with Nonminimal Derivative Coupling of Scalar Field Agus Suroso and Freddy P. Zen Theoretical Physics Laboratory,
More informationLOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS.
LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS Merab Gogberashvili a and Paul Midodashvili b a Andronikashvili Institute of Physics, 6 Tamarashvili Str., Tbilisi 3877, Georgia E-mail: gogber@hotmail.com
More informationBrane in the Relativistic Theory of Gravitation
Brane in the Relativistic Theory of Gravitation arxiv:gr-qc/0009v Jan 00 Ramy Naboulsi March 0, 008 Tokyo Institute of Technology, Department of Physics, O-Okoyama, Meguro-ku, Tokyo Abstract It was proven
More informationElementary/Composite Mixing in Randall-Sundrum Models
Elementary/Composite Mixing in Randall-Sundrum Models Brian Batell University of Minnesota with Tony Gherghetta - arxiv:0706.0890 - arxiv:0710.1838 Cornell 1/30/08 5D Warped Dimension = 4D Strong Dynamics
More informationBrane Gravity from Bulk Vector Field
Brane Gravity from Bulk Vector Field Merab Gogberashvili Andronikashvili Institute of Physics, 6 Tamarashvili Str., Tbilisi 380077, Georgia E-mail: gogber@hotmail.com September 7, 00 Abstract It is shown
More informationNeutron Stars in the Braneworld
Neutron Stars in the Braneworld Mike Georg Bernhardt Ruprecht-Karls-Universität Heidelberg Zentrum für Astronomie, Landessternwarte 24 April 29 Outline Introduction Why bother with Extra Dimensions? Braneworlds
More informationCritical exponents in quantum Einstein gravity
Critical exponents in quantum Einstein gravity Sándor Nagy Department of Theoretical physics, University of Debrecen MTA-DE Particle Physics Research Group, Debrecen Leibnitz, 28 June Critical exponents
More informationTime-Like Extra Dimension and Cosmological Constant in Brane Models. Tianjun Li
UPR-901-T Time-Like Extra Dimension and Cosmological Constant in Brane Models Tianjun Li Department of Physics and Astronomy University of Pennsylvania, Philadelphia, PA 19104-6396 U. S. A. Abstract We
More informationNon-SUSY BSM: Lecture 1/2
Non-SUSY BSM: Lecture 1/2 Generalities Benasque September 26, 2013 Mariano Quirós ICREA/IFAE Mariano Quirós (ICREA/IFAE) Non-SUSY BSM: Lecture 1/2 1 / 31 Introduction Introduction There are a number of
More informationWarped Brane-worlds in 6D Flux Compactification
Warped Brane-worlds in D Flux Compactification Lefteris Papantonopoulos National Technical University of Athens Plan of the Talk Brane-worlds Why -Dimensions? Codimension-1 branes Codimension- branes D
More informationHIGGS-GRAVITATIONAL INTERATIONS! IN PARTICLE PHYSICS & COSMOLOGY
HIGGS-GRAVITATIONAL INTERATIONS! IN PARTICLE PHYSICS & COSMOLOGY beyond standard model ZHONG-ZHI XIANYU Tsinghua University June 9, 015 Why Higgs? Why gravity? An argument from equivalence principle Higgs:
More informationFriedmann Equation in Codimension-two Braneworlds
Friedmann Equation in Codimension-two Braneworlds Chen Fang Master of Science Department of Physics McGill University Montréal, Québec, Canada September 1, 2007 A thesis submitted to McGill University
More informationSUPERSTRING REALIZATIONS OF SUPERGRAVITY IN TEN AND LOWER DIMENSIONS. John H. Schwarz. Dedicated to the memory of Joël Scherk
SUPERSTRING REALIZATIONS OF SUPERGRAVITY IN TEN AND LOWER DIMENSIONS John H. Schwarz Dedicated to the memory of Joël Scherk SOME FAMOUS SCHERK PAPERS Dual Models For Nonhadrons J. Scherk, J. H. Schwarz
More informationCosmology and astrophysics of extra dimensions
Cosmology and astrophysics of extra dimensions Astrophysical tests of fundamental physics Porto, 27-29 March 2007 P. Binétruy, APC Paris Why extra dimensions? Often appear in the context of unifying gravitation
More informationκ = f (r 0 ) k µ µ k ν = κk ν (5)
1. Horizon regularity and surface gravity Consider a static, spherically symmetric metric of the form where f(r) vanishes at r = r 0 linearly, and g(r 0 ) 0. Show that near r = r 0 the metric is approximately
More informationCompositeness at ILC250?
Compositeness at ILC250? F. Richard LAL-Orsay International workshop on future linear colliders LCWS Strasbourg 23-27 October 2017 F. Richard LAL-Orsay October 2017 1 Introduction There are various interpretations
More informationString Theory II GEORGE SIOPSIS AND STUDENTS
String Theory II GEORGE SIOPSIS AND STUDENTS Department of Physics and Astronomy The University of Tennessee Knoxville, TN 37996-1200 U.S.A. e-mail: siopsis@tennessee.edu Last update: 2006 ii Contents
More informationAlternatives to the GUT Seesaw
Alternatives to the GUT Seesaw Motivations Higher-dimensional operators String instantons Other (higher dimensions, Higgs triplets) Motivations Many mechanisms for small neutrino mass, both Majorana and
More informationCosmology with Extra Dimensions
Cosmology with Extra Dimensions Johannes Martin University of Bonn May 13th 2005 Outline Motivation and Introduction 1 Motivation and Introduction Motivation From 10D to 4D: Dimensional Reduction Common
More informationModelling an extra dimension with domain-wall branes
Modelling an extra dimension with domain-wall branes Damien George Nikhef theory seminar 5 th November 2009 Overview Physics beyond the standard model: extra dimensions. Brane domain wall (topological
More informationVanishing Dimensions in Four Dimensional Cosmology with Nonminimal Derivative Coupling of Scalar Field
Advanced Studies in Theoretical Physics Vol. 9, 2015, no. 9, 423-431 HIKARI Ltd, www.m-hikari.com http://dx.doi.org/10.12988/astp.2015.5234 Vanishing Dimensions in Four Dimensional Cosmology with Nonminimal
More informationFromBigCrunchToBigBang IsItPossible? Nathan Seiberg School of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA.
hep-th/0201039 FromBigCrunchToBigBang IsItPossible? Nathan Seiberg School of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA seiberg@ias.edu ABSTRACT We discuss the possibility of
More informationNeutrinos & Large Extra Dimensions. Renata Zukanovich Funchal Universidade de São Paulo, Brazil
Neutrinos & Large Extra Dimensions Renata Zukanovich Funchal Universidade de São Paulo, Brazil What is ν? Workshop June 26, 2012 ν Masses & Mixings Majorana CP Violating phases solar atmospheric accelerator
More informationg ab dx a dx b b 2 d τ 2, (1)
COSMOLOGICAL VARIATION OF THE SCALAR FIELD AND ISOCHRONAL GEODESICS IN NON-COMPACTIFIED KALUZA THEORY L.L. Williams Konfluence Research Institute ABSTRACT Classical, non-compactified five-dimensional Kaluza
More informationCLASSIFICATION OF 5D WARPED SPACES WITH COSMOLOGICAL CONSTANT
CLASSIFICATION OF 5D WARPED SPACES WITH COSMOLOGICAL CONSTANT AUREL BEJANCU Department of Mathematics Kuwait University, Kuwait E-mail:aurel.bejancu@ku.edu.kw CONSTANTIN CĂLIN Department of Mathematics
More informationExotic Dark Matter as Spin-off of Proton Stability. Kaustubh Agashe (University of Maryland)
Exotic Dark Matter as Spin-off of Proton Stability Kaustubh Agashe (University of Maryland) Outline and Summary Warped extra dimensions address Planckweak and flavor hierarchies: new (KK) particles at
More informationarxiv:hep-ph/ v3 9 Jan 2002
SNUTP 01-046 May 27, 2017 Self-tuning Solution of Cosmological Constant in RS-II Model and Goldstone Boson arxiv:hep-ph/0112344v3 9 Jan 2002 Jihn E. Kim 1 Department of Physics and Center for Theoretical
More informationTachyon scalar field in DBI and RSII cosmological context
Tachyon scalar field in DBI and RSII cosmological context Neven Bilic, Goran S. Djordjevic, Milan Milosevic and Dragoljub D. Dimitrijevic RBI, Zagreb, Croatia and FSM, University of Nis, Serbia 9th MATHEMATICAL
More informationParticle Physics and Cosmology II: Dark Matter
Particle Physics and Cosmology II: Dark Matter Mark Trodden Center for Particle Cosmology University of Pennsylvania Second Lecture Puerto Vallarta Mexico 1/13/2011 Problems of Modern Cosmology Is cosmic
More informationSearch for Randall-Sundrum Gravitons and Intermediate-Mass Diphoton Resonances
Search for Randall-Sundrum Gravitons and Intermediate-Mass Diphoton Resonances (CMS Draft Analysis Note) V. Litvin, H. Newman, T. Orimoto, E. Schneider California Institute of Technology, Pasadena, CA,
More informationSupersymmetric Randall-Sundrum Scenario
CIT-USC/00-015 Supersymmetric Randall-Sundrum Scenario arxiv:hep-th/000117v May 000 Richard Altendorfer, Jonathan Bagger Department of Physics and Astronomy The Johns Hopkins University 400 North Charles
More informationCosmology of moving branes and spinflation
Cosmology of moving branes and spinflation 8 Dark Energy in the Universe Damien Easson University of Tokyo Outline Brane Inflation, Moduli Stabilization and Flux Compactifications Cyclic, Mirage cosmologies
More informationElectroweak Symmetry Breaking via Strong Dynamics in the Precision Higgs Era: Extra Dimension and Composite Higgs.
Electroweak Symmetry Breaking via Strong Dynamics in the Precision Higgs Era: Extra Dimension and Composite Higgs Tirtha Sankar Ray XXI DAE-BRNS HEP Symposium, 8-12 December, 2014 The Standard Model All
More informationString Theory I Mock Exam
String Theory I Mock Exam Ludwig Maximilians Universität München Prof. Dr. Dieter Lüst 15 th December 2015 16:00 18:00 Name: Student ID no.: E-mail address: Please write down your name and student ID number
More informationThe Higgs Mechanism and the Higgs Particle
The Higgs Mechanism and the Higgs Particle Heavy-Ion Seminar... or the Anderson-Higgs-Brout-Englert-Guralnik-Hagen-Kibble Mechanism Philip W. Anderson Peter W. Higgs Tom W. B. Gerald Carl R. François Robert
More informationThe Influence of DE on the Expansion Rate of the Universe and its Effects on DM Relic Abundance
The Influence of DE on the Expansion Rate of the Universe and its Effects on DM Relic Abundance Esteban Jimenez Texas A&M University XI International Conference on Interconnections Between Particle Physics
More informationOddities of the Universe
Oddities of the Universe Koushik Dutta Theory Division, Saha Institute Physics Department, IISER, Kolkata 4th November, 2016 1 Outline - Basics of General Relativity - Expanding FRW Universe - Problems
More informationarxiv: v1 [gr-qc] 3 Oct 2015
Vacuum expectation value profiles of the bulk scalar field in the generalized Rall-Sundrum model A. Tofighi a, 1 M. Moazzen b, A. Farokhtabar a arxiv:1510.00790v1 [gr-qc] 3 Oct 2015 a Department of Physics,
More informationHow to tell apart non-standard EWSB mechanisms. Veronica Sanz CERN and YORK Moriond 2012
How to tell apart non-standard EWSB mechanisms Veronica Sanz CERN and YORK Moriond 2012 In this talk What is standard? EWSB by elementary scalar(s) includes SM and SUSY What is non-standard? EWSB by -composite
More informationHolographic self-tuning of the cosmological constant
Holographic self-tuning of the cosmological constant Francesco Nitti Laboratoire APC, U. Paris Diderot IX Crete Regional Meeting in String Theory Kolymbari, 10-07-2017 work with Elias Kiritsis and Christos
More informationAdS/CFT duality. Agnese Bissi. March 26, Fundamental Problems in Quantum Physics Erice. Mathematical Institute University of Oxford
AdS/CFT duality Agnese Bissi Mathematical Institute University of Oxford March 26, 2015 Fundamental Problems in Quantum Physics Erice What is it about? AdS=Anti de Sitter Maximally symmetric solution of
More informationarxiv:gr-qc/ v1 29 Jan 2003
Some properties of a string V. Dzhunushaliev June, 8 Dept. Phys. and Microel. Engineer., KRSU, Bishkek, Kievskaya Str., 7, Kyrgyz Republic arxiv:gr-qc/38v 9 Jan 3 Abstract The properties of 5D gravitational
More informationAttractor Structure of Gauged Nambu-Jona-Lasinio Model
Attractor Structure of Gauged ambu-jona-lasinio Model Department of Physics, Hiroshima University E-mail: h-sakamoto@hiroshima-u.ac.jp We have studied the inflation theory in the gauged ambu-jona-lasinio
More informationExtra Dimensional Signatures at CLIC
Extra Dimensional Signatures at CLIC Thomas G. Rizzo SLAC A brief overview is presented of the signatures for several different models with extra dimensions at CLIC, an e + e linear collider with a center
More information