- •1. Introduction
- •2. Supersymmetry essentials
- •2.1. A new spacetime symmetry
- •2.2. Supersymmetry and the weak scale
- •2.3. The neutral supersymmetric spectrum
- •2.4. R-Parity
- •2.5. Supersymmetry breaking and dark energy
- •2.6. Minimal supergravity
- •2.7. Summary
- •3. Neutralino cosmology
- •3.1. Freeze out and wimPs
- •3.2. Thermal relic density
- •3.2.1. Bulk region
- •1. Introduction
- •2. Construction of trial functions
- •2.1. A new formulation of perturbative expansion
- •2.2. Trial function for the quantum double-well potential
- •3. Hierarchy theorem and its generalization
- •4. Asymmetric quartic double-well problem
- •4.1. Construction of the first trial function
- •4.2. Construction of the second trial function
- •4.3. Symmetric vs asymmetric potential
- •5. The n-dimensional problem
- •1. Introduction
- •2. The star product formalism
- •3. Geometric algebra and the Clifford star product
- •4. Geometric algebra and classical mechanics
- •5. Non-relativistic quantum mechanics
- •6. Spacetime algebra and Dirac theory
- •7. Conclusions
- •1. Introduction
- •1.1. Historical overview
- •1.2. Aims of this article
- •2. Random curves and lattice models
- •2.1. The Ising and percolation models
- •2.1.1. Exploration process
- •2.2. O (n) model
- •2.3. Potts model
- •2.4. Coulomb gas methods
- •2.4.1. Winding angle distribution
- •2.4.2. N-leg exponent
- •3.1. The postulates of sle
- •3.2. Loewner’s equation
- •3.3. Schramm–Loewner evolution
- •3.4. Simple properties of sle
- •3.4.1. Phases of sle
- •3.4.2. Sle duality
- •3.5. Special values of κ
- •3.5.1. Locality
- •3.5.2. Restriction
- •3.6. Radial sle and the winding angle
- •3.6.1. Identification with lattice models
- •4. Calculating with sle
- •4.1. Schramm’s formula
- •4.2. Crossing probability
- •4.3. Critical exponents from sle
- •4.3.1. The fractal dimension of sle
- •4.3.2. Crossing exponent
- •4.3.3. The one-arm exponent
- •5. Relation to conformal field theory
- •5.1. Basics of cft
- •5.2. Radial quantisation
- •5.3. Curves and states
- •5.4. Differential equations
- •5.4.1. Calogero–Sutherland model
- •6. Related ideas
- •6.1. Multiple slEs
- •6.2. Other variants of sle
- •6.3. Other growth models
- •1. Introduction
- •1.1. Acoustic force field
- •1.2. Primary axial acoustic force
- •1.3. Primary and secondary acoustic force
- •2. Application of Newton’s second law
- •3. Mathematical model
- •3.1. Preliminary analysis
- •4. Equation for particle trajectories
- •5. Concentration equation
- •6. Experimental procedure and results
- •6.1. SiC particle trajectories in an acoustic field
- •7. Comparison between experimental results and mathematical model
- •8. Summary and conclusions
3.2. Thermal relic density
We now want to apply the general formalism above to the specific case of neutralinos. This is complicated by the fact that neutralinos may annihilate to many final states: , W+W−, ZZ, Zh, hh, and states including the heavy Higgs bosons H, A, and H±. Many processes contribute to each of these final states, and nearly every supersymmetry parameter makes an appearance in at least one process. The full set of annihilation diagrams is discussed in [18]. Codes to calculate the relic density are publicly available [19].
Given this complicated picture, it is not surprising that there are a variety of ways to achieve the desired relic density for neutralino dark matter. What is surprising, however, is that many of these different ways may be found in minimal supergravity, provided one looks hard enough. We will therefore consider various regions of minimal supergravity parameter space where qualitatively distinct mechanisms lead to neutralino dark matter with the desired thermal relic density.
3.2.1. Bulk region
As evident from Fig. 6, the LSP is a Bino-like neutralino in much of minimal supergravity parameter space. It is useful, therefore, to begin by considering the pure Bino limit. In this case, all processes with final state gauge bosons vanish. This follows from supersymmetry and the absence of 3-gauge boson vertices involving the hypercharge gauge boson.
The process through a t-channel sfermion does not vanish in the Bino limit. This process is the first shown in Fig. 8. This reaction has an interesting structure. Recall that neutralinos are Majorana fermions. If the initial state neutralinos are in an S-wave state, the Pauli exclusion principle implies that the
New ways to solve the Schroedinger equation
R. Friedberg and T.D. Lee aDepartment of Physics, Columbia University, New York, NY 10027, USA bChina Center of Advanced Science and Technology (CCAST) (World Laboratory), P.O. Box 8730, Beijing 100080, People’s Republic of China cRIKEN BNL Research Center (RBRC), Brookhaven National Laboratory, Upton, NY 11973, USA Received 27 July 2004; accepted 5 August 2004. Available online 15 December 2004.
Abstract
We discuss a new approach to solve the low lying states of the Schroedinger equation. For a fairly large class of problems, this new approach leads to convergent iterative solutions, in contrast to perturbative series expansions. These convergent solutions include the long standing difficult problem of a quartic potential with either symmetric or asymmetric minima.
Article Outline
1. Introduction
2. Construction of trial functions
2.1. A new formulation of perturbative expansion
2.2. Trial function for the quantum double-well potential
3. Hierarchy theorem and its generalization
4. Asymmetric quartic double-well problem
4.1. Construction of the first trial function
4.2. Construction of the second trial function
4.3. Symmetric vs asymmetric potential
5. The N-dimensional problem
Appendix A. A soluble example
A.1. A two-level model
A.2. Square-well example (Cont.)
A.3. The iterative sequence
References