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Friday, 5 July 2013

The Measurement Problem, Part 1

The Problem


The measurement problem becomes a problem only when we neglect to specify the nature of the observer's Hilbert space. Postulates I (Systems are described by vectors in a Hilbert space) and II (Time evolution occurs via some given Hamiltonian for a particular system) are fine in that regard. These two postulates deal only with the description of a quantum system. It is the third postulate (Measurement leads to collapse of state vector to an eigenstate) where there is a problem.

A measurement is said to occur whenever one quantum system - the "observer" - described by a Hilbert space ( $ H_{O} $ ) interacts with another system described by a Hilbert space ($H_{S}$). The complete Hilbert space of the system ("observer" and the "observed") is given by:
$$ H_{O+S} = H_{O} \otimes H_{S} $$
To actually realize the dichotomy between an "internal" and "external" observer, the size of the observer's Hilbert space, given by its dimension ($dim(H_O)$), must be comparable to ($dim(H_S)$) - the dimension of the Hilbert space corresponding to the system under observation. Instead, what we generally encounter is ($dim(H_O) \gg dim(H_S)$) as is the case for, say, an apparatus with a vacuum chamber and other paraphernalia which is being used to study an atomic scale sample.

In this case the apparatus is not described by the three states ($\{\ket{ready}, \ket{up}, \ket{down}\}$), but by the larger family of states ($\{\ket{ready;\alpha}, \ket{up;\alpha}, \ket{down;\alpha}$) where ($\alpha$) parametrizes the "helper" degrees of freedom of the apparatus which are not directly involved in generating the final output, but are nevertheless present in any interaction. Examples of these d.o.f are the states of the electrons in the wiring which transmits data between the apparatus and the system.

The initial state of the complete system is of the form:
$$\ket{\psi_i} = \ket{ready;\alpha} (\mu \ket{1} + \nu \ket{0} )$$
When $ H_O$ interacts with $ H_S$ in such a way, that a measurement is said to have occurred, the final state of the composite system can be written as:
$$\ket{\psi_i} = \ket{up;\alpha} (\mu_{up} \ket{1} + \nu_{up} \ket{0}) + \ket{down;\alpha} (\mu_{down} \ket{1} + \nu_{down} \ket{0})$$
In a complete self-consistent theory, one would hope that all paradoxes regarding measurement could be resolved by understanding unitary evolution of the full Hilbert space ($H_{sum}$). This is not quite the case. Consider the case when the system being observed is a spin-1/2 object with a two dimensional Hilbert space ($H_{sys}$) a basis for which can be written as ($\{ \ket{0}; \ket{1} \} $). The Hilbert space of the observing apparatus ($H_{obs}$) is large enough to describe all the possible positions of dials, meters and probes on the apparatus. Let us assume that ($H_{obs}$) can itself be written as a tensor product:
$$H_{obs} = H_{pointer} \otimes H_{res}$$
For some poorly understood reason, when ($N_{obs} \rightarrow \infty$), an interaction between the two systems - observer and subject - causes the state of the subject to "collapse" to one of the eigenstates of the operator (or "property") of the subject being measured ($\ket{\psi_{sub}} \rightarrow \ket{\phi^i_{obs}}$).

When QM was first invented, it was understood that the measuring apparatus is a classical system requiring an infinite number of degrees of freedom for its complete description. Thus the ``collapse'' that occurs is because of something that happens at the interface of the classical measuring apparatus and the quantum system being observed. This ad-hoc separation of the classical from the quantum came to known as the "Heisenberg cut" (or "Bohr cut" depending of your reading of history). Since the quantum description of systems with even a few degrees of freedom appeared to be a great technical feat in those early days, physicists didn't have much reason to worry about systems with large ($N \gg 1$) dimension Hilbert spaces.

Mechanisms for Wavevector Collapse


To address the lack of understanding of state vector collapse in QM, and to get a grasp on the description of systems with large Hilbert spaces, first the many-worlds interpretation (MWI) and later the consistent histories or decoherence framework was constructed.

Monday, 11 February 2013

Thermal Time and Kepler's Second Law

In a fascinating recent paper (arXiv:1302.0724), Haggard and Rovelli (HR) discuss the relationship between the concept of thermal time, the Tolman-Ehrenfest effect and the rate of dynamical evolution of a system - i.e., the number of distinguishable (orthogonal) states a given system transitions through in each unit of time. The last of these is also the subject of the Margolus-Levitin theorem (arXiv:quant-ph/9710043v2) according to which the rate of dynamical evolution of a macroscopic system with fixed average energy (E), has an upper bound ($\nu_{\perp}$) given by:

\begin{equation}
\label{eqn:margolus-levitin}
\nu_{\perp} \leq \frac{2E}{h}
\end{equation}

Thursday, 31 January 2013

Some things ... cannot be learned quickly

There are some things which cannot be learned quickly,
and time, which is all we have,
must be paid heavily for their acquiring.
They are the very simplest things,
and because it takes a man’s life to know them
the little new that each man gets from life
is very costly and the only heritage he has to leave.

- Ernest Hemingway (From A. E. Hotchner, Papa Hemingway, Random House, NY, 1966)

Sunday, 27 January 2013

Elementary particles and quantum geometry

Black holes are formed due to the gravitational collapse of matter - ordinary matter, consisting of the particles and excitations of the Standard Model that we know and love. These include electrons, photons, neutrinos, quarks, mesons etc, and their respective anti-particles. General Relativity tells us that the properties of (macroscopic) black holes are universal, in that they do not depend on the precise fraction of each particle species in the initial "mixture".

A black hole formed from the collapse of a non-rotating cloud of $ n$ electrons and $ n$ positrons will be neutral, non-rotating and of mass $ 2n m_e$, where $ m_e$ is the electron mass. Let us refer to this black hole as $ bh(n,e^-; n,e^+)$ or $ bh_e$ for short. A black hole formed from the collapse of cloud of $ m$ neutrinos and $ m$ anti-neutrinos, where $ m * m_{\nu} = n * m_e$ ($ m_{\nu}$ being the mass of a neutrino). According to our labeling scheme, this black hole will be labeled as $ bh(m,\nu;m,\bar\nu)$ or $ bh_{\nu}$ for short. Both black holes have the same mass $ M = n * m_e = m * m_{\mu} $ and thus the same horizon area $ A = GM/c^2$.

... and so it begins

Welcome to my blog, gentle readers. Here you will be exposed to all manner of speculation and conjecture on my part. Those with an enhanced sensitivity to non-rigorous reasoning might occasionally experience a feeling akin to motion sickness. I urge such rigor-bound passengers to depart at the earliest exit. To the rest, welcome aboard. Happy trails!