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This structure can be read with a Perl CGI. The script has some funkiness from metacharacters in the plist, and when I wrote this script, I used the -best-possible-way=false flag:

We write the number of space-time dimensions as D = n + 4, where we understand that the n dimensions which contract are all spatial and the remaining dimensions are 3 + 1 dimensional space-time The metric can be written in a general form which is split between time, the expanding dimensions, and the contracting dimensions as D 1 2 3 ds 2 = dt 2 + a 2 (t ) dxi2 + b 2 (t ) dx m m=4 i =1 (1610).

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Some addresses are reserved for specific purposes. A HOST_ID of 0 is reserved to identify an entire subnetwork. For example, the address 168.152.20.0 refers to a Class C address with a NET_ID of 168.152.20. A HOST_ID that consists of all ones (usually written 255 when referring to an all-ones byte, but also denoted as -1 ) is reserved as a broadcast address and is used to transmit a message to all hosts on a particular network.

Levin, Janna, In ation from Extra Dimensions, Phys. Lett. vol. B343, 1995, 69 75.

One of the most valuable but least understood tools in IP protocol management is called the subnet mask. Subnet masks are used to identify the portion of the address that specifies the network or the subnetwork for routing purposes. They also may be used to divide a large address into subnetworks or to combine multiple, smaller addresses to create a single large domain. In the case of an organization subdividing its network, the address space is apportioned to identify multiple logical networks. This is accomplished by further dividing the HOST_ID subfield into a Subnetwork Identifier (SUBNET_ID) and a HOST_ID.

% cat test.cgi #!/usr/bin/perl use Mac::PropertyList::SAX qw( parse_plist ); use CGI; my $q = CGI->new; print $q->header(); print $q->start_html('Your Title Here'); $r = $q->Dump; $r $r $r $r =~ =~ =~ =~ s/\</</g; s/\>/>/g; s/\"/\'/g; s/<br \/>//g;

As soon as the Internet became popular in the early 90s, concerns began to arise about the eventual exhaustion of available IP addresses. For example, consider what happens when a small corporation of 11 employees purchases a Class C address. They now control more than 250 addresses, of which they may only be using 25. Clearly, this is a waste of a scarce resource. One technique that has been accepted for address space conservation is called Classless Interdomain Routing (CIDR). CIDR effectively limits the number of addresses assigned to a given organization, making the process of address assignment far more granular and therefore efficient. Furthermore, CIDR has had a secondary, yet equally important, impact: It has dramatically reduced the size of the Internet routing tables because of the preallocation techniques used for address space management.

Here, a(t) is a scale factor associated with the three expanding spatial dimensions and b(t) is a scale factor associated with the contracting spatial dimensions. Solving the Einstein equations in vacuum gives the following: a b 3 +n =0 a b a k ( 3) + 2( H a + nH b ) H a + 2 2 = 0 a a b n 1 + (3H a + ( n 1) H b ) H b + 2 k ( n ) = 0 b b Here we have introduced two Hubble constants. One is the usual Hubble constant associated with our expanding universe Ha: Ha = a a (16.11)

if ($r =~ /<\!DOCTYPE plist PUBLIC/) { $r = $&.$'; if ($r =~ /<\/plist>/) { $r = $`.$&; } } my $data = parse_plist( $r );

Downloaded from Digital Engineering Library @ McGraw-Hill (www.digitalengineeringlibrary.com) Copyright 2004 The McGraw-Hill Companies. All rights reserved. Any use is subject to the Terms of Use as given at the website.

The second Hubble constant is associated with the contracting extra dimensions: Hb = b b (16.12)

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$vals = $$data{'parameters'}; for ($idx = 0; $idx < scalar(@$vals);$idx++) { print "coord[".$idx."] = (".$$vals[$idx]{'targetX'}.", ".$$vals[$idx]{'targetY'}.")".$q->br; }

The constants k(3) and k(n) are related to the local curvature and so can be +1, 0, 1. We choose the locally at case and so set k(3) = k(n) = 0. This allows the equations to be simpli ed somewhat, giving three relations for the Hubble constants:

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