The news that Mexican physicist Arturo Menchaca and
archaeologist Linda Manzanilla have launched a cosmic
muon search for hidden chambers in the Pyramid of
the Sun in Mexico (Physics
Today, February 2004, page 31) opens a new and
exciting chapter in cross−disciplinary research.
The two researchers have chosen the technique of pyramid
probing with vertical muons—that is, those making
an angle less than 45° to zenith. Vertical muons
were first used in 1955 in Australia (ref. 5 of ref.
1). Luis Alvarez and coworkers used the method in
their 1967−68 probing of Chephren's pyramid,
the second of the great pyramids of Egypt. The Alvarez
team searched for equivalents of the king's and queen's
chambers that had been found in the first pyramid,
that of Chephren's father, Cheops.
The vertical muon probing method consists of measuring,
from beneath the pyramid, the absorption pattern of
the muons as a function of their angle to zenith after
they pass through the pyramid. The detector was placed
in the only known chamber beneath Chephren's pyramid.
As a result of the probing, Alvarez concluded that
no other chamber existed.1
"It's not that we did not find the chamber," said
Alvarez. "We found that there wasn't any chamber."2
Menchaca and Manzanilla appear to be unaware of
an article by two French architects3
that was published two decades after Alvarez's investigation.
In describing their search for cavities in the Cheops
pyramid, the architects pointed out an important construction
feature, unknown to Alvarez at the time of his search,
that brings into question the feasibility of observing
hidden chambers from beneath the pyramids.
Alvarez assumed that the pyramids were filled with
only one kind of stone—limestone—so that
their interior density is uniform. The architects
reported that the Cheops pyramid was built of two
kinds of stone with different densities: limestone,
at 1.8 g/cm2, and granite, at 2.7 g/cm2.
While most of the first pyramid's interior consists
of limestone, the roofs and walls of all chambers
and galleries are made of granite. The mass of the
granite roof above the king's chamber is equal, within
5%, to the sum of the missing mass of the chamber
plus the mass of the roof if it were made of limestone;4
the apparent area density of the king's chamber, as
detected by the vertical muons, approximately equals
that of limestone. By accident or by design, the excess
density of granite over that of the limestone nearly
exactly masks the void. Had Alvarez first tested his
system in the Cheops pyramid, from beneath, he could
not have detected the king's chamber with vertical
muons.
Are these considerations, based solely on our knowledge
of the Cheops pyramid, valid for Chephren's as well?
They would be invalid if Chephren's pyramid was built
without granite. However, the lower chamber's granite
roof suggests that no such radical departure in architecture
took place between the father's pyramid and the son's.
I first saw the French architects' article3
in January 1987 while in Cairo filming a documentary
about the pyramids.2
I immediately informed Alvarez of the French group's
findings. He confirmed that he was unaware of the
use of granite in the pyramids.
I suggested to Alvarez that to unambiguously state
that there are no other chambers in Chephren's pyramid,
one would have to repeat the measurement using horizontal
muons—those that make an angle greater than
45° to zenith—and that the detector should
be on the ground outside the pyramid.5
The intensity of the horizontal muons is much lower
than that of the vertical ones, but the horizontal
muons have the advantage of being "hardened" by their
longer passage through the atmosphere. In fact, Alvarez's
experiment1 had confirmed
the feasibility of using horizontal muons: The muon
absorption pattern had clearly shown the ridges of
the peak of the Cheops pyramid viewed from the Chephren
pyramid's lower chamber.
In a letter written to me less than a year before
his death, Alvarez stood by his conclusion that no
king's or queen's chambers exist in Chephren's pyramid.
He argued that if a hypothetical king's chamber had
included a granite roof, his detector would have observed
it as a density bump. Because no such bump was observed,
Chephren's pyramid must have been constructed differently
from Cheops's. Alvarez did tacitly imply, however,
that the issue was not closed; he said another measurement,
using horizontal muons, would confirm his conclusion.
Actually, the issue is wide open, because the only
chamber found in the Chephren pyramid was built like
all chambers in the Cheops pyramid—with a granite
roof. To exclude the existence of chambers in the
Chephren pyramid, an experiment with horizontal muons
is called for.
How is this story relevant to the Pyramid of the
Sun? If the Mexican pyramid's interior density is
homogeneous, it will be irrelevant. If the density
is not homogeneous, the story may be quite relevant.
According to the Physics Today story, Menchaca says
the Pyramid of the Sun has a more irregular shape,
is less dense, and is also less homogeneous.
References
1. L. W. Alvarez et al., Science
167, 832 (1970); see also L. Alvarez, Adventures
in Exp. Phys. 1, 157 (1972).
2. Tesla Foundation, Unfolding Pyramids'
Secrets Using Modern Physics, film, narrated by
L. W. Alvarez and B. C. Maglich, directed by Victoria
Vesna (1988).
3. J. Lakshmanan, J. Montlucon, Geophys.:
The Leading Edge 6, 10 (1987).
4. Joint ARE−USA Research Team,
Electromagnetic Sounder Experiments at the Pyramids
of Giza, NSF doc. no. GF−38767, Ain Shams
U., Cairo, Egypt, and SRI, Menlo Park, CA (May 1975).
See also I. E. S. Edwards, The Pyramids of Egypt,
Penguin Books, New York (1985).
Menchaca comments: The account by Bogdan
C. Maglich on unpublished details of the Chephren
pyramid experiment by Luis Alvarez and coworkers1
provides fascinating insight into this pioneering
application of high−energy physics to archaeology.
The method used by Alvarez involves finding statistically
significant differences between measured and simulated
muon flows in a given direction. The necessary ignorance
of a detailed density distribution inside the investigated
volume requires an approximation. As Maglich implies,
both we and the Alvarez group assumed that the internal
pyramid density is constant. Also, we are aware2
of the limitations introduced, not only by uncertainties
related to the internal density distribution, but
also by uncertainties about the external shape description,
among other factors.
In Teotihuacan we assume that the mean composition
and density distribution are similar to those found
inside a 200−meter−long horizontal tunnel
excavated near the base of the Pyramid of the Sun
last century. We sampled the pyramid filling along
that tunnel. The study reveals that the Mexican monument,
although fairly uniform, is more heterogeneous than
the Egyptian pyramid seems to be as judged by the
limestone walls of the tunnel leading to the Belzoni
chamber, where the Alvarez team located its muon detector.
The measured mean density in Teotihuacan turns out
to be appreciably smaller than the density of rock.
As Maglich correctly suggests, we do consider the
conditions in which stony walls of a hypothetical
hidden cavity would result in a compensated mean density
that would cancel the sought−for signal. This
and other considerations helped determine the limitations
of our experiment.2
In contrast with the Chephren case, archaeological
excavations in the Pyramid of the Sun provide excellent
calibration references. Finally, in the Egyptian case,
we tend to agree with the private response Maglich
says he received from Alvarez concerning the unlikely
possibility that a cavity having a granite ceiling
would result in mean density compensation in all directions.
That would be particularly unlikely with internal
structures as large and intricate as those found in
the Cheops pyramid.
References
1. L. W. Alvarez et al., Science
167, 832 (1970).
2. R. Alfaro et al., Rev. Mex. Fis.
49(S4), 54 (2003).