21
Yuri Kamyshkov email: [email protected] UT P599 Particle and Cosmology seminar January 25, 2017 Based on the work in collaboration with B. Kerbikov (ITEP), Y. K., L. Varriano (UT) 1

Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: [email protected] UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

  • Upload
    others

  • View
    0

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

Yuri Kamyshkovemail: [email protected]

UT P599 Particle and Cosmology seminar • January 25, 2017

Based on the work in collaboration with B. Kerbikov (ITEP), Y. K., L. Varriano (UT)

1

Page 2: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

http://en.wikipedia.org/wiki/Two-state_quantum_system

Examples: - electron spin precession in mag. filed- NMR- Chemistry

In Particle Physics: - neutral ↔ oscillations- neutrino flavor oscillations- oscillations of →- oscillation of → mirror state

2

Page 3: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

:

3

Page 4: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

In general Hamiltonian with mixing leads to oscillations between two components. E.g. neutron oscillation when :

Hamiltonian isHermitian matrix unitary

Oscillation frequency 4

Page 5: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

5Probability doesn’t depend on E but on .

Page 6: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

There are more general description with density matrix

• L. D. Landau and E. M. Lifshitz, Quantum Mechanics, Course Theoretical Physics v. 3 • R. P. Feynman, Statistical Mechanics, A Set Of Lectures (Advanced Books Classics)• https://en.wikipedia.org/wiki/Density_matrix

Mixedstate: ′ = 10 + 01 ; + = 1| ˃ = 10 ; | ˃ = 01= ∗ ∗∗ ∗ = −density matrix

= − · = − +

Liouville–von Neumann equation for density matrix evolution

( = 0) = 1 00 06

Page 7: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

Hamiltonian can be more complex, e.g. for the oscillating neutron moving through the gas (no mag. field)

Real potential diff.increases frequency

Absorptiondamping

Proper oscillation

Frequency ofthe system

we should expect for frequency:

7

=

Page 8: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

For even more general case of the complex potential, decay, and including magnetic field and spin:

System of 16 coupled diff. eqs can be handled by Mathematica

8

Page 9: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

9

Page 10: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

10

Thi description by Liouville–von Neumann equation is still not complete

Direct interaction with environment via incoherent elastic collisions is not included. This will lead to decoherence.

http://www.nybooks.com/articles/2017/01/19/trouble-with-quantum-mechanics/

“Most general evolution of probabilities satisfies an equation of a class known as Lindblad equations.”

= − · = − + − Liouville–von Neumann equation

Page 11: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

This equation includes in general the loss of coherence of oscillating system to environment.

Loss of coherence is the reset of the oscillation phase between two components.At this moment oscillating system collapses (with some probability) into one of its pure states and continue motion with this boundary conditions. It is “measurement” of the system by the environment; system remains in the oscillating state with reset boundary conditions.

11

https://en.wikipedia.org/wiki/Lindblad_equation

Page 12: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

Example of decoherence of two-level system in old classical paper

m+

e-

m-

e+

Measurement of the system (the effect):decaywithemissionofMichel s ;or inelastic collision with molecules leading again to the decay of the

Here the evolution equation for has resulted into simple form of Lindblad equation 12

Page 13: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

13

Page 14: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

(1)

14

Page 15: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

(2)

15

Page 16: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

(1)

(2)

16

Page 17: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

It looks like the Lindblad “super-operator” term is coming here from the incoherent elastic scattering of oscillating system on the molecules of environment.

17

Page 18: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

… and produces a decoherence effect on oscillation.

Probability of oscillation in vacuum

18

Page 19: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

∗∗

Scattering Integral in Feinberg & Weinberg evolution equation

= ( ) 00 ( )

Will be zero if one of f’s is zero

Source of decoherence

19

Page 20: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

Loss of COHERENCE is due to scattering integral

t

mea

sure

men

t

0M

PP

N=

In the vacuum the probability coherently grows as ~ [ ( ) ] . Every incoherent elastic collision resets the oscillating system’s phase to zero, but the system continues its motion in the environment contributing (with + sign) to the evolution of until it is being “measured” at some later time.Weinberg’s recommendation is to make number of collisions < 1. That is the reason why current muoniumoscillation search experiments are being performed in vacuum or with zero pressure.

Absorption and decaymake here negative contribution

20

Page 21: Yuri Kamyshkov - UTK Department of Physics and Astronomy€¦ · Yuri Kamyshkov email: kamyshkov@utk.edu UT P599 Particle and Cosmology seminar • January 25, 2017 Based on the work

Loss of coherence in transformation?• In ESS n-nbar experiment with L=200-m vacuum vessel and residual pressure is <10

or < 10 ,vacuum gas H2 , with total cross section 82 barns for thermal neutrons (overestimate), the probability of elastic collision for the neutron component with gas molecules is ≲ 10 per flight. Elastic x-section for component is not well known but its x-section is not larger than for .• If incoherent elastic scattering will occur to oscillating system in the beam, the

system will be scattered isotropically in s-wave and will be mostly removed from the beam. So it will not contribute to the evolution of matrix through scattering integral, since the system after scattering can not be measured.

Conclusion: for oscillation in gas with residual pressure < 10 the evolution equation has the form :

without scattering integral introducing decoherence. 21