The Matter Content of the Standard Model (SM) Consists of Three Families of Chiral Quarks and Leptons. Each Family Has Five Diff

Total Page:16

File Type:pdf, Size:1020Kb

The Matter Content of the Standard Model (SM) Consists of Three Families of Chiral Quarks and Leptons. Each Family Has Five Diff I. SUPERSYMMETRIC GRAND UNIFICATION A. Supersymmetrizing the standard model: particle content The matter content of the standard model (SM) consists of three families of chiral quarks and leptons. Each family has five different gauge representations: qL(3, 2)+1/6, uR(3¯, 1)−2/3, dR(3¯, 1)+1/3, lL(1, 2)−1/2, eR(1, 1)+1. (1) 1 All of these fields are Weyl fermions that transform in the ( 2 , 0) representation of the Lorentz group (they have an undotted spinor index α). The subscripts R, L do not specify the repre- sentation of the Lorentz group but instead are used to indicate the different transformation properties under the SU(2)L gauge group. In addition, there is a single scalar representation, that is the Higgs field: h(1, 2)−1/2. (2) As we learned in the previous section, supersymmetry requires the presence of additional states which form supermultiplets with the known particles. Since all states of a super- multiplet carry the same gauge quantum numbers, we need at least a doubling of states: For every field of the SM, one has to postulate a superpartner with the exact same gauge quantum numbers and a spin such that it can form an appropriate supermultiplet. More specifically, the quarks and leptons are promoted to chiral supermultiplets by adding scalar I I ˜I ˜I I (spin-0) squarks (˜qL,u ˜R, dR) and sleptons (lL,e ˜R) to the spectrum. The gauge bosons 1 ˜ ˜ ˜ are promoted to vector multiplets by adding the corresponding spin- 2 gauginos (G, W , B) to the spectrum. Finally, the Higgs boson is also promoted to a chiral multiplet with a 1 spin- 2 Higgsino superpartner. However, the supersymmetric version of the SM cannot ‘live’ with only one Higgs doublet and at least a second doublet, of opposite hypercharge, has to be added. This can be seen from the fact that one cannot write down a supersymmetric version of the Yukawa interactions of the SM without introducing a second Higgs doublet. The reason is the definite chirality of the Higgsino. Another way to see the necessity of a second Higgs doublet is the fact that the Higgsino is a chiral fermion which carries U(1) hypercharge and hence it upsets the anomaly cancellation condition. A second Higgsino of opposite U(1)Y charge is necessary. 1 B. Gauge coupling unification There is an interesing conclusion that follows from the quantum number assignments of the new particles that we have introduced to make the SM supersymmetric. An attractive feature of the SM is that the quarks and leptons of each generation fill out multiplets of the simple gauge group SU(5). This suggests a very beautiful picture, called grand unification, in which SU(5), or a group such as SO(10) or E6 for which SU(5) is a subgroup, is the fundamental gauge symmetry at very short distances. This unified symmetry is spontaneously broken to the SM gauge group SU(3) × SU(2) × U(1). For definiteness, we focus on SU(5). The generators of SU(5) can be represented as 5× 5 Hermitian matrices acting on the 5-dimensional vectors in the fundamental representations. To see how the SM is embedded in SU(5), it is convenient to write these matrices as block with 3 and 2 rows and columns. Then, the SM generators can be identified as 1 ta 0 3 − 1 SU(3) : ; SU(2) : ; U(1) : 3 . (3) 1 ! a ! s5 1 ! 0 σ /2 2 a a A B 1 AB The matrices t and σ /2 are normalized to tr[T T ] = 2 δ , while the last matrix is identifed with 3/5 Y . The symmetryq breaking can be caused by the VEV of a Higgs fields in the adjoint representation of SU(5). The VEV − 1 1 hΦi = V · 3 (4) 1 1 ! 2 commutes with the generators in (3) but not with the off-diagonal generators. It thus breaks SU(5) → SU(3) × SU(2) × U(1). Matter fermions can be organized as left-handed Weyl fermions in the SU(5) representa- tions 5¯ and 10, where the latter is the antisymmetric matrix: d¯ 0u ¯ u¯ u d d¯ 0u ¯ u d 5¯ : d¯ ; 10: 0 u d . (5) e 0e ¯ ν 0 The SU(5) covariant derivative is A A Dm = ∂m − ig5AmT , (6) 2 where g5 is the SU(5) gauge coupling. There is only room for one value here. So this model predicts that the three SM gauge couplings are related by g3 = g2 = g1 = g5, (7) where 5 ′ g3 = gs, g2 = g, g1 = g . (8) s3 ′ To test this picture, we must check whether the measured values of gs,g,g evolve at very short distances into values that obey (7). 2 gi Let αi = 4π for i = 1, 2, 3. The one-loop renormalization group equations for the gauge couplings are dg b dα b i = − i g3 or i = − i α2. (9) d log Q (4π)2 i d log Q 2π i For U(1), the coefficient b1 is 2 3 1 3 b = − Y 2 − Y 2, (10) 1 3 5 f 3 5 b Xf Xb where the two sums run over multiplets of left-handed Weyl fermions (f) and complex- 3 2 valued bosons (b). The factors 5 Y are the squares of the U(1) charges defined by (3). For non-Abelian groups, the b-coefficients are 11 2 1 b = C (G) − C(r ) − C(r ), (11) 3 2 3 f 3 b Xf Xb where C2(G) and C(r) are the standard group theory coefficients. For SU(N), 1 C (G)= C(G)= N, C(N)= . (12) 2 2 The solution of the RGE (9) is − − b Q α 1(Q)= α 1(M)+ i log . (13) i i 2π M Now consider the situation where the three couplings gi become equal at the mass scale MU , the mass scale of the SU(5) symmetry breaking. Using (13), we can then determine the SM couplings at any lower mass scale. The three αi(Q) are determined by two parameters. We can thus eliminate those parameters and obtain the relation −1 −1 −1 α3 = (1+ B)α2 − Bα1 , (14) 3 where b − b B = 3 2 . (15) b2 − b1 The values of the αi are known very accurately at Q = mZ : −1 −1 −1 α3 =8.50 ± 0.14, α2 = 29.57 ± 0.02, α1 = 59.00 ± 0.02. (16) Inserting these values into (14), we find B =0.716 ± 0.005 ± 0.03. (17) The first error is that propagated from the errors in (16). The second is an estimate of the systematic error from neglecting the two-loop renormalization group coefficients and other higher-order corrections. We can compare the value of B in (17) to the values of (15) from different models. The hypothesis that the three SM gauge couplings unify is acceptable only if the gauge theory that describes physics between mZ and MU gives a value of B consistent with (17). The minimal SM fails this test: • SU(3): each fermion generation has four triplets. The Higgs fields are color singlets. • SU(2): each fermion generation has four doublets. The Higgs fields are doublets. • U(1): Each fermion generation have Y 2 = 6(1/6)2 + 3(2/3)2 + 3(1/3)2 + 2(1/2)2 + 1(1)2 = 10/3. Each Higgs doublet hasP Y 2 = 2(1/2)2 =1/2. P Thus, the SM values of the bi are 4 b = 11 − n , 3 3 g 22 4 1 b = − n − n , 2 3 3 g 6 h 4 1 b = − n − n , (18) 1 3 g 10 h where ng is the number of generations and nh is the number of Higgs doublets. Notice that ng cancels out of (15). This is to be expected. The SM fermions form complete representations of SU(5), and so their renormalization effects cannot lead to differences among the three couplings. For the SM with any number of generations and any number of Higgs doublets, we have (11/3)+(1/6)nh BMHDM(ng, nh)= . (19) (22/3) − (1/15)nh 4 For the minimal SM, with nh = 1, we have 115 B = =0.528, (20) SM 218 35 far away from (17). To get a value consistent with (17) we need nh = 6: B6HDM = 52 =0.673. We can redo the calculation in the minimal supersymmetric version of the SM (SSM). First of all, we should rewrite (11) for a supersymmetric model with one vector supermul- tiplet, containing a vector and a Weyl fermion in the adjoint representation, and a set of chiral supermultiplets indexed by k, each with a Weyl fermion and a complex boson. Then (11) becomes 11 2 2 1 b = C (G) − C (G) − + C(r ) i 3 2 3 2 3 3 k Xk = 3C2(G) − C(rk). (21) Xk The formula (22) undergoes a similar rearrangement: 3 b = − Y 2. (22) 1 5 k Xk For a supersymmetric model with ng generations and nh Higgs doublets, we have b3 = 9 − 2ng, 1 b = 6 − 2n − n , 2 g 2 h 3 b = −2n − n . (23) 1 g 10 h The SSM has nh = 2, yielding 5 B = =0.714, (24) SSM 7 in excellent agreement with (17). Actually, the results here overstate the case for supersymmetry by ignoring two-loop terms in the RGEs, and also by integrating these equations all the way down to mZ , even though, from searches at high energy colliders, most of the squarks and gluinos must be heavier than 300 GeV.
Recommended publications
  • Supersymmetric Dark Matter
    Supersymmetric dark matter G. Bélanger LAPTH- Annecy Plan | Dark matter : motivation | Introduction to supersymmetry | MSSM | Properties of neutralino | Status of LSP in various SUSY models | Other DM candidates z SUSY z Non-SUSY | DM : signals, direct detection, LHC Dark matter: a WIMP? | Strong evidence that DM dominates over visible matter. Data from rotation curves, clusters, supernovae, CMB all point to large DM component | DM a new particle? | SM is incomplete : arbitrary parameters, hierarchy problem z DM likely to be related to physics at weak scale, new physics at the weak scale can also solve EWSB z Stable particle protect by symmetry z Many solutions – supersymmetry is one best motivated alternative to SM | NP at electroweak scale could also explain baryonic asymetry in the universe Relic density of wimps | In early universe WIMPs are present in large number and they are in thermal equilibrium | As the universe expanded and cooled their density is reduced Freeze-out through pair annihilation | Eventually density is too low for annihilation process to keep up with expansion rate z Freeze-out temperature | LSP decouples from standard model particles, density depends only on expansion rate of the universe | Relic density | A relic density in agreement with present measurements (Ωh2 ~0.1) requires typical weak interactions cross-section Coannihilation | If M(NLSP)~M(LSP) then maintains thermal equilibrium between NLSP-LSP even after SUSY particles decouple from standard ones | Relic density then depends on rate for all processes
    [Show full text]
  • Quantum Field Theory*
    Quantum Field Theory y Frank Wilczek Institute for Advanced Study, School of Natural Science, Olden Lane, Princeton, NJ 08540 I discuss the general principles underlying quantum eld theory, and attempt to identify its most profound consequences. The deep est of these consequences result from the in nite number of degrees of freedom invoked to implement lo cality.Imention a few of its most striking successes, b oth achieved and prosp ective. Possible limitation s of quantum eld theory are viewed in the light of its history. I. SURVEY Quantum eld theory is the framework in which the regnant theories of the electroweak and strong interactions, which together form the Standard Mo del, are formulated. Quantum electro dynamics (QED), b esides providing a com- plete foundation for atomic physics and chemistry, has supp orted calculations of physical quantities with unparalleled precision. The exp erimentally measured value of the magnetic dip ole moment of the muon, 11 (g 2) = 233 184 600 (1680) 10 ; (1) exp: for example, should b e compared with the theoretical prediction 11 (g 2) = 233 183 478 (308) 10 : (2) theor: In quantum chromo dynamics (QCD) we cannot, for the forseeable future, aspire to to comparable accuracy.Yet QCD provides di erent, and at least equally impressive, evidence for the validity of the basic principles of quantum eld theory. Indeed, b ecause in QCD the interactions are stronger, QCD manifests a wider variety of phenomena characteristic of quantum eld theory. These include esp ecially running of the e ective coupling with distance or energy scale and the phenomenon of con nement.
    [Show full text]
  • Quantum Statistics: Is There an Effective Fermion Repulsion Or Boson Attraction? W
    Quantum statistics: Is there an effective fermion repulsion or boson attraction? W. J. Mullin and G. Blaylock Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003 ͑Received 13 February 2003; accepted 16 May 2003͒ Physicists often claim that there is an effective repulsion between fermions, implied by the Pauli principle, and a corresponding effective attraction between bosons. We examine the origins and validity of such exchange force ideas and the areas where they are highly misleading. We propose that explanations of quantum statistics should avoid the idea of an effective force completely, and replace it with more appropriate physical insights, some of which are suggested here. © 2003 American Association of Physics Teachers. ͓DOI: 10.1119/1.1590658͔ ␺ ͒ϭ ͒ Ϫ␣ Ϫ ϩ ͒2 I. INTRODUCTION ͑x1 ,x2 ,t C͕f ͑x1 ,x2 exp͓ ͑x1 vt a Ϫ␤͑x ϩvtϪa͒2͔Ϫ f ͑x ,x ͒ The Pauli principle states that no two fermions can have 2 2 1 ϫ Ϫ␣ Ϫ ϩ ͒2Ϫ␤ ϩ Ϫ ͒2 the same quantum numbers. The origin of this law is the exp͓ ͑x2 vt a ͑x1 vt a ͔͖, required antisymmetry of the multi-fermion wavefunction. ͑1͒ Most physicists have heard or read a shorthand way of ex- pressing the Pauli principle, which says something analogous where x1 and x2 are the particle coordinates, f (x1 ,x2) ϭ ͓ Ϫ ប͔ to fermions being ‘‘antisocial’’ and bosons ‘‘gregarious.’’ Of- exp imv(x1 x2)/ , C is a time-dependent factor, and the ten this intuitive approach involves the statement that there is packet width parameters ␣ and ␤ are unequal.
    [Show full text]
  • A Generalization of the One-Dimensional Boson-Fermion Duality Through the Path-Integral Formalsim
    A Generalization of the One-Dimensional Boson-Fermion Duality Through the Path-Integral Formalism Satoshi Ohya Institute of Quantum Science, Nihon University, Kanda-Surugadai 1-8-14, Chiyoda, Tokyo 101-8308, Japan [email protected] (Dated: May 11, 2021) Abstract We study boson-fermion dualities in one-dimensional many-body problems of identical parti- cles interacting only through two-body contacts. By using the path-integral formalism as well as the configuration-space approach to indistinguishable particles, we find a generalization of the boson-fermion duality between the Lieb-Liniger model and the Cheon-Shigehara model. We present an explicit construction of n-boson and n-fermion models which are dual to each other and characterized by n−1 distinct (coordinate-dependent) coupling constants. These models enjoy the spectral equivalence, the boson-fermion mapping, and the strong-weak duality. We also discuss a scale-invariant generalization of the boson-fermion duality. arXiv:2105.04288v1 [quant-ph] 10 May 2021 1 1 Introduction Inhisseminalpaper[1] in 1960, Girardeau proved the one-to-one correspondence—the duality—between one-dimensional spinless bosons and fermions with hard-core interparticle interactions. By using this duality, he presented a celebrated example of the spectral equivalence between impenetrable bosons and free fermions. Since then, the one-dimensional boson-fermion duality has been a testing ground for studying strongly-interacting many-body problems, especially in the field of integrable models. So far there have been proposed several generalizations of the Girardeau’s finding, the most promi- nent of which was given by Cheon and Shigehara in 1998 [2]: they discovered the fermionic dual of the Lieb-Liniger model [3] by using the generalized pointlike interactions.
    [Show full text]
  • 1 Standard Model: Successes and Problems
    Searching for new particles at the Large Hadron Collider James Hirschauer (Fermi National Accelerator Laboratory) Sambamurti Memorial Lecture : August 7, 2017 Our current theory of the most fundamental laws of physics, known as the standard model (SM), works very well to explain many aspects of nature. Most recently, the Higgs boson, predicted to exist in the late 1960s, was discovered by the CMS and ATLAS collaborations at the Large Hadron Collider at CERN in 2012 [1] marking the first observation of the full spectrum of predicted SM particles. Despite the great success of this theory, there are several aspects of nature for which the SM description is completely lacking or unsatisfactory, including the identity of the astronomically observed dark matter and the mass of newly discovered Higgs boson. These and other apparent limitations of the SM motivate the search for new phenomena beyond the SM either directly at the LHC or indirectly with lower energy, high precision experiments. In these proceedings, the successes and some of the shortcomings of the SM are described, followed by a description of the methods and status of the search for new phenomena at the LHC, with some focus on supersymmetry (SUSY) [2], a specific theory of physics beyond the standard model (BSM). 1 Standard model: successes and problems The standard model of particle physics describes the interactions of fundamental matter particles (quarks and leptons) via the fundamental forces (mediated by the force carrying particles: the photon, gluon, and weak bosons). The Higgs boson, also a fundamental SM particle, plays a central role in the mechanism that determines the masses of the photon and weak bosons, as well as the rest of the standard model particles.
    [Show full text]
  • 7. Gamma and X-Ray Interactions in Matter
    Photon interactions in matter Gamma- and X-Ray • Compton effect • Photoelectric effect Interactions in Matter • Pair production • Rayleigh (coherent) scattering Chapter 7 • Photonuclear interactions F.A. Attix, Introduction to Radiological Kinematics Physics and Radiation Dosimetry Interaction cross sections Energy-transfer cross sections Mass attenuation coefficients 1 2 Compton interaction A.H. Compton • Inelastic photon scattering by an electron • Arthur Holly Compton (September 10, 1892 – March 15, 1962) • Main assumption: the electron struck by the • Received Nobel prize in physics 1927 for incoming photon is unbound and stationary his discovery of the Compton effect – The largest contribution from binding is under • Was a key figure in the Manhattan Project, condition of high Z, low energy and creation of first nuclear reactor, which went critical in December 1942 – Under these conditions photoelectric effect is dominant Born and buried in • Consider two aspects: kinematics and cross Wooster, OH http://en.wikipedia.org/wiki/Arthur_Compton sections http://www.findagrave.com/cgi-bin/fg.cgi?page=gr&GRid=22551 3 4 Compton interaction: Kinematics Compton interaction: Kinematics • An earlier theory of -ray scattering by Thomson, based on observations only at low energies, predicted that the scattered photon should always have the same energy as the incident one, regardless of h or • The failure of the Thomson theory to describe high-energy photon scattering necessitated the • Inelastic collision • After the collision the electron departs
    [Show full text]
  • Higgsino DM Is Dead
    Cornering Higgsino at the LHC Satoshi Shirai (Kavli IPMU) Based on H. Fukuda, N. Nagata, H. Oide, H. Otono, and SS, “Higgsino Dark Matter in High-Scale Supersymmetry,” JHEP 1501 (2015) 029, “Higgsino Dark Matter or Not,” Phys.Lett. B781 (2018) 306 “Cornering Higgsino: Use of Soft Displaced Track ”, arXiv:1910.08065 1. Higgsino Dark Matter 2. Current Status of Higgsino @LHC mono-jet, dilepton, disappearing track 3. Prospect of Higgsino Use of soft track 4. Summary 2 DM Candidates • Axion • (Primordial) Black hole • WIMP • Others… 3 WIMP Dark Matter Weakly Interacting Massive Particle DM abundance DM Standard Model (SM) particle 500 GeV DM DM SM Time 4 WIMP Miracle 5 What is Higgsino? Higgsino is (pseudo)Dirac fermion Hypercharge |Y|=1/2 SU(2)doublet <1 TeV 6 Pure Higgsino Spectrum two Dirac Fermions ~ 300 MeV Radiative correction 7 Pure Higgsino DM is Dead DM is neutral Dirac Fermion HUGE spin-independent cross section 8 Pure Higgsino DM is Dead DM is neutral Dirac Fermion Purepure Higgsino Higgsino HUGE spin-independent cross section 9 Higgsino Spectrum (with gaugino) With Gauginos, fermion number is violated Dirac fermion into two Majorana fermions 10 Higgsino Spectrum (with gaugino) 11 Higgsino Spectrum (with gaugino) No SI elastic cross section via Z-boson 12 [N. Nagata & SS 2015] Gaugino induced Observables Mass splitting DM direct detection SM fermion EDM 13 Correlation These observables are controlled by gaugino mass Strong correlation among these observables for large tanb 14 Correlation These observables are controlled by gaugino mass Strong correlation among these observables for large tanb XENON1T constraint 15 Viable Higgsino Spectrum 16 Current Status of Higgsino @LHC 17 Collider Signals of DM p, e- DM DM is invisible p, e+ DM 18 Collider Signals of DM p, e- DM DM is invisible p, e+ DM Additional objects are needed to see DM.
    [Show full text]
  • Glossary of Scientific Terms in the Mystery of Matter
    GLOSSARY OF SCIENTIFIC TERMS IN THE MYSTERY OF MATTER Term Definition Section acid A substance that has a pH of less than 7 and that can react with 1 metals and other substances. air The mixture of oxygen, nitrogen, and other gasses that is consistently 1 present around us. alchemist A person who practices a form of chemistry from the Middle Ages 1 that was concerned with transforming various metals into gold. Alchemy A type of science and philosophy from the Middle Ages that 1 attempted to perform unusual experiments, taking something ordinary and turning it into something extraordinary. alkali metals Any of a group of soft metallic elements that form alkali solutions 3 when they combine with water. They include lithium, sodium, potassium, rubidium, cesium, and francium. alkaline earth Any of a group of metallic elements that includes beryllium, 3 metals magnesium, calcium, strontium, barium, and radium. alpha particle A positively charged particle, indistinguishable from a helium atom 5, 6 nucleus and consisting of two protons and two neutrons. alpha decay A type of radioactive decay in which a nucleus emits 6 an alpha particle. aplastic anemia A disorder of the bone marrow that results in too few blood cells. 4 apothecary The person in a pharmacy who distributes medicine. 1 atom The smallest component of an element that shares the chemical 1, 2, 3, 4, 5, 6 properties of the element and contains a nucleus with neutrons, protons, and electrons. atomic bomb A bomb whose explosive force comes from a chain reaction based on 6 nuclear fission. atomic number The number of protons in the nucleus of an atom.
    [Show full text]
  • BCS Thermal Vacuum of Fermionic Superfluids and Its Perturbation Theory
    www.nature.com/scientificreports OPEN BCS thermal vacuum of fermionic superfuids and its perturbation theory Received: 14 June 2018 Xu-Yang Hou1, Ziwen Huang1,4, Hao Guo1, Yan He2 & Chih-Chun Chien 3 Accepted: 30 July 2018 The thermal feld theory is applied to fermionic superfuids by doubling the degrees of freedom of the Published: xx xx xxxx BCS theory. We construct the two-mode states and the corresponding Bogoliubov transformation to obtain the BCS thermal vacuum. The expectation values with respect to the BCS thermal vacuum produce the statistical average of the thermodynamic quantities. The BCS thermal vacuum allows a quantum-mechanical perturbation theory with the BCS theory serving as the unperturbed state. We evaluate the leading-order corrections to the order parameter and other physical quantities from the perturbation theory. A direct evaluation of the pairing correlation as a function of temperature shows the pseudogap phenomenon, where the pairing persists when the order parameter vanishes, emerges from the perturbation theory. The correspondence between the thermal vacuum and purifcation of the density matrix allows a unitary transformation, and we found the geometric phase associated with the transformation in the parameter space. Quantum many-body systems can be described by quantum feld theories1–4. Some available frameworks for sys- tems at fnite temperatures include the Matsubara formalism using the imaginary time for equilibrium systems1,5 and the Keldysh formalism of time-contour path integrals3,6 for non-equilibrium systems. Tere are also alterna- tive formalisms. For instance, the thermal feld theory7–9 is built on the concept of thermal vacuum.
    [Show full text]
  • Baryon and Lepton Number Anomalies in the Standard Model
    Appendix A Baryon and Lepton Number Anomalies in the Standard Model A.1 Baryon Number Anomalies The introduction of a gauged baryon number leads to the inclusion of quantum anomalies in the theory, refer to Fig. 1.2. The anomalies, for the baryonic current, are given by the following, 2 For SU(3) U(1)B , ⎛ ⎞ 3 A (SU(3)2U(1) ) = Tr[λaλb B]=3 × ⎝ B − B ⎠ = 0. (A.1) 1 B 2 i i lef t right 2 For SU(2) U(1)B , 3 × 3 3 A (SU(2)2U(1) ) = Tr[τ aτ b B]= B = . (A.2) 2 B 2 Q 2 ( )2 ( ) For U 1 Y U 1 B , 3 A (U(1)2 U(1) ) = Tr[YYB]=3 × 3(2Y 2 B − Y 2 B − Y 2 B ) =− . (A.3) 3 Y B Q Q u u d d 2 ( )2 ( ) For U 1 BU 1 Y , A ( ( )2 ( ) ) = [ ]= × ( 2 − 2 − 2 ) = . 4 U 1 BU 1 Y Tr BBY 3 3 2BQYQ Bu Yu Bd Yd 0 (A.4) ( )3 For U 1 B , A ( ( )3 ) = [ ]= × ( 3 − 3 − 3) = . 5 U 1 B Tr BBB 3 3 2BQ Bu Bd 0 (A.5) © Springer International Publishing AG, part of Springer Nature 2018 133 N. D. Barrie, Cosmological Implications of Quantum Anomalies, Springer Theses, https://doi.org/10.1007/978-3-319-94715-0 134 Appendix A: Baryon and Lepton Number Anomalies in the Standard Model 2 Fig. A.1 1-Loop corrections to a SU(2) U(1)B , where the loop contains only left-handed quarks, ( )2 ( ) and b U 1 Y U 1 B where the loop contains only quarks For U(1)B , A6(U(1)B ) = Tr[B]=3 × 3(2BQ − Bu − Bd ) = 0, (A.6) where the factor of 3 × 3 is a result of there being three generations of quarks and three colours for each quark.
    [Show full text]
  • Introduction to Supersymmetry
    Introduction to Supersymmetry Pre-SUSY Summer School Corpus Christi, Texas May 15-18, 2019 Stephen P. Martin Northern Illinois University [email protected] 1 Topics: Why: Motivation for supersymmetry (SUSY) • What: SUSY Lagrangians, SUSY breaking and the Minimal • Supersymmetric Standard Model, superpartner decays Who: Sorry, not covered. • For some more details and a slightly better attempt at proper referencing: A supersymmetry primer, hep-ph/9709356, version 7, January 2016 • TASI 2011 lectures notes: two-component fermion notation and • supersymmetry, arXiv:1205.4076. If you find corrections, please do let me know! 2 Lecture 1: Motivation and Introduction to Supersymmetry Motivation: The Hierarchy Problem • Supermultiplets • Particle content of the Minimal Supersymmetric Standard Model • (MSSM) Need for “soft” breaking of supersymmetry • The Wess-Zumino Model • 3 People have cited many reasons why extensions of the Standard Model might involve supersymmetry (SUSY). Some of them are: A possible cold dark matter particle • A light Higgs boson, M = 125 GeV • h Unification of gauge couplings • Mathematical elegance, beauty • ⋆ “What does that even mean? No such thing!” – Some modern pundits ⋆ “We beg to differ.” – Einstein, Dirac, . However, for me, the single compelling reason is: The Hierarchy Problem • 4 An analogy: Coulomb self-energy correction to the electron’s mass A point-like electron would have an infinite classical electrostatic energy. Instead, suppose the electron is a solid sphere of uniform charge density and radius R. An undergraduate problem gives: 3e2 ∆ECoulomb = 20πǫ0R 2 Interpreting this as a correction ∆me = ∆ECoulomb/c to the electron mass: 15 0.86 10− meters m = m + (1 MeV/c2) × .
    [Show full text]
  • The Standard Model and Beyond Maxim Perelstein, LEPP/Cornell U
    The Standard Model and Beyond Maxim Perelstein, LEPP/Cornell U. NYSS APS/AAPT Conference, April 19, 2008 The basic question of particle physics: What is the world made of? What is the smallest indivisible building block of matter? Is there such a thing? In the 20th century, we made tremendous progress in observing smaller and smaller objects Today’s accelerators allow us to study matter on length scales as short as 10^(-18) m The world’s largest particle accelerator/collider: the Tevatron (located at Fermilab in suburban Chicago) 4 miles long, accelerates protons and antiprotons to 99.9999% of speed of light and collides them head-on, 2 The CDF million collisions/sec. detector The control room Particle Collider is a Giant Microscope! • Optics: diffraction limit, ∆min ≈ λ • Quantum mechanics: particles waves, λ ≈ h¯/p • Higher energies shorter distances: ∆ ∼ 10−13 cm M c2 ∼ 1 GeV • Nucleus: proton mass p • Colliders today: E ∼ 100 GeV ∆ ∼ 10−16 cm • Colliders in near future: E ∼ 1000 GeV ∼ 1 TeV ∆ ∼ 10−17 cm Particle Colliders Can Create New Particles! • All naturally occuring matter consists of particles of just a few types: protons, neutrons, electrons, photons, neutrinos • Most other known particles are highly unstable (lifetimes << 1 sec) do not occur naturally In Special Relativity, energy and momentum are conserved, • 2 but mass is not: energy-mass transfer is possible! E = mc • So, a collision of 2 protons moving relativistically can result in production of particles that are much heavier than the protons, “made out of” their kinetic
    [Show full text]