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Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about.

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Presentation on theme: "Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about."— Presentation transcript:

1 Grand Unified Theory, Running Coupling Constants and the Story of our Universe
These next theories are in a less rigorous state and we shall talk about them, keeping in mind that they are at the ‘”edge” of what is understood today. Nevertheless, they represent a qualitative view of our universe, from the perspective of particle physics and cosmology. GUT -- Grand Unified Theories – symmetry between quarks and leptons; decay of the proton. Running coupling constants: it’s possible that at one time in the development of the universe all the forces had the same strength The Early Universe: a big bang, cooling and expanding, phase transitions and broken symmetries

2 Grand Unified Theory (GUT)
We have incorporated into the Lagrangian density invariance under rotations in U(1)XSU(2)flavor space and SU(3)color space, but these were not really unified. That is, the gauge bosons, (photon, W, and Z, and gluons) were not manifestations of the same force field. If one were to “unify” these fields, how might it occur? The attempts to do so are called Grand Unified Theories. Grand Unified Theory (GUT) GUT includes invariance under U(1) X SU(2)flavor space and SU(3)color and invariance under the following transformations: quarks  leptons leptons  quarks

3 e-i(x,y,t) ; Grand Unified Theory - SU(5) d red dgreen d blue e- -
Georgii & Glashow, Phys. Rev Lett. 32, 438 (1974). mx  1015GeV Quarks & leptons in same multiplet 8 gluons d red rgb dgreen 24 Gauge bosons ; L d blue (W 0+B) W+ e- - W- (W 0 +B) Left handed L SU(5) is invariant under SU(5) gau Gauge invariance e-i(x,y,t) For symmetry under SU(5), the x and y particles must be massless!

4 i D = - i g5/2j=1,24jXi where Xi = the 24 gauge bosons
SU(5) generators and covariant derivative i The = generators of SU(5) are the 5x5 matrices which i(x,y,t) has do not commute. SU(5) is a non-abelian local gauge theory. 24 components: i(x,y,t) = all real, continuous functions D = - i g5/2j=1,24jXi where Xi = the 24 gauge bosons This includes the Standard Model covariant derivative (couplings are different). Predictions: a) qup = 2/3 ; qd = -1/3 b) sin2W  0.23 c) the proton decays! > years d) baryon number not conserved e) only one coupling constant, g5 (g1, g2, and g3, are related) So far, there is no evidence that the proton decays. But note that the lifetime of the universe is 14 billion years. The probability of detecting a decaying proton depends a large sample of protons!

5 “Particle Physics and Cosmology”,
P.D. B. Collins, A. D. Martin and E. J. Squires, Wiley, NY, page 169

6 B The term j =1,2,…,24jXi /2 can be written: _ | |_ _ | _| 24 . g5
same as SU(3)color _ | |_ _ | _| B 24 . same as SU(2)flavor this matrix X comes in 3 color states with |Q| = 4/3 y comes in 3 color states with |Q| = 1/3 g5

7 The GUT SU(5) Lagrangian density (1st generation only)
Standard Model terms g5 int. SU(5)

8 - - X +  = 1,2,3 Q = - 4/3 Y  Q= - 1/3  = 1,2,3
3-color vertex quark to lepton, no color change  = 1,2,3 Q = - 4/3 - Y  3-color vertex quark to lepton, no color change Q= - 1/3  = 1,2,3 + Hermitian Conjugate (contains X+ and Y+ terms) Note: one coupling constant, g5 T  transpose Charge conjugation operator

9 proton, SU(5)  1031 years -- a great failure for SU(5)
a great failure of SU(5)!

10 charge dred X-4/3red e+ e+

11 - e+ Decay of proton in SU(5) - Xred proton X +red d red d red u green
anti-up - u green d red - green Xred u blue X+ red blue e+ 3-color vertex proton X +red green blue

12 Supergravity SUPER SYMMETRIC (SUSY) THEORIES:
SUSYs contain invariance of the Lagrangian density under operations which change bosons (spin = 01,2,..) fermions (spin = ½, 3/2 …). SUSY  unifies E&M, weak, strong (SU(3) and gravity fields. usually includes invariance under local transformations Supergravity

13 Supersymmetric String Theories
Elementary particles are one-dimensional strings: open strings closed strings .no free parameters or L = 2r L = cm. = Planck Length Mplanck  GeV/c2 See Schwarz, Physics Today, November 1987, p. 33 “Superstrings” The Planck Mass is approximately that mass whose gravitational potential is the same strength as the strong QCD force at r  cm. An alternate definition is the mass of the Planck Particle, a hypothetical miniscule black hole whose Schwarzchild radius is equal to the Planck Length.

14 A quick way to estimate the Planck mass is as follows:
gstrong ℏc/r = GMpMp/r where r = 10-15cm (strong force range) and gstrong = 1 Mp = [gstrong ℏc/G]1/2 = x 1019 mproton MPlanck  GeV/c2

15 Up to 10 – 43 seconds after the Big Bang
Particle Physics and the Development of the Universe Very early universe All ideas concerning the very early universe are speculative. No accelerator experiments probe energies of sufficient magnitude to provide any experimental insight into the behavior of matter at the energy levels that prevailed during this period. Planck epoch Up to 10 – 43 seconds after the Big Bang At the energy levels that prevailed during the Planck epoch the four fundamental forces— electromagnetism U(1) , gravitation, weak SU(2), and the strong SU(3) color — are assumed to all have the same strength, and “unified” in one fundamental force. Little is known about this epoch. Theories of supergravity/ supersymmetry, such as string theory, are candidates for describing this era.

16 Grand unification epoch: GUT
Between 10–43 seconds and 10–36 seconds after the Big Bang The universe expands and cools from the Planck epoch. After about 10–43 seconds the gravitational interactions are no longer unified with the electromagnetic U(1) , weak SU(2), and the strong SU(3) color interactions. Supersymmetry/Supergravity symmetires are broken. After 10–43 seconds the universe enters the Grand Unified Theory (GUT) epoch. A candidate for GUT is SU(5) symmetry. In this realm the proton can decay, quarks are changed into leptons and all the gauge particles (X,Y, W, Z, gluons and photons), quarks and leptons are massless. The strong, weak and electromagnetic fields are unified.

17 Running Coupling Constants
Electro weak unification Planck region Electro- Weak Symmetry breaking Super- symmetry SU(3) GUT electroweak GeV

18 Inflation and Spontaneous Symmetry Breaking.
At about 10–36 seconds and an average thermal energy kT  1015 GeV, a phase transition is believed to have taken place. In this phase transition, the vacuum state undergoes spontaneous symmetry breaking. Spontaneous symmetry breaking: Consider a system in which all the spins can be up, or all can be down – with each configuration having the same energy. There is perfect symmetry between the two states and one could, in theory, transform the system from one state to the other without altering the energy. But, when the system actually selects a configuration where all the spins are up, the symmetry is “spontaneously” broken.

19 Higgs Mechanism When the phase transition takes place the vacuum state transforms into a Higgs particle (with mass) and so-called Goldstone bosons with no mass. The Goldstone bosons “give up” their mass to the gauge particles (X and Y gain masses 1015 GeV). The Higgs keeps its mass ( the thermal energy of the universe, kT 1015 GeV). This Higgs particle has too large a mass to be seen in accelerators. What causes the inflation? The universe “falls into” a low energy state, oscillates about the minimum (giving rise to the masses) and then expands rapidly. When the phase transition takes place, latent heat (energy) is released. The X and Y decay into ordinary particles, giving off energy. It is this rapid expansion that results in the inflation and gives rise to the “flat” and homogeneous universe we observe today. The expansion is exponential in time.

20 R eHt Schematic of Inflation R(t) m T (GeV/k) Rt2/3 1019 Rt1/2
T t-1/2 R eHt 1014 T t-1/2 Rt1/2 Tt-2/3 T=2.7K 10-13 10-43 10-34 10-31 time (sec) 10

21 Electroweak epoch Between 10–36 seconds and 10–12 seconds after the Big Bang The SU(3) color force is no longer unified with the U(1)x SU(2) weak force. The only surviving symmetries are: SU(3) separately, and U(1)X SU(2). The W and Z are massless. A second phase transition takes place at about 10–12 seconds at kT = 100 GeV. In this phase transition, a second Higgs particle is generated with mass close to 100 GeV; the Goldstone bosons give up their mass to the W, Z and the particles (quarks and leptons). It is the search for this second Higgs particle that is thought to have been detected at LHC.

22 After the Big Bang: the first 10-6 Seconds
W , Z0 take on mass inflation X,Y take on mass gravity decouples Planck Era . SUSY Supergravity GUT SU(2) x U(1) symmetry . all forces unified bosons  fermions . quarks  leptons all particles massless

23 W , Z0 take on mass 2.7K Standard Model . . atoms formed . .
COBE data . 2.7K Standard Model 100Gev . . . only gluons and photons are massless . atoms formed n, p formed nuclei formed .

24 Field theoretic treatment of the Higgs mechanism
One can incorporate the Higgs mechanism into the Lagrangian density by including scalar fields for the vacuum state. When the scalar fields undergo a gauge transformation, they generate the particle masses. The Lagrangian density is then no longer gauge invariant. The symmetry is broken.

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