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Structure and Evolution of Online Social Networks

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70% in Flickr and 84% in Yahoo! 360. How does density change with time? Degree distribution ... Flickr Contacts. Component sizes in. 360 Contacts. How do ... – PowerPoint PPT presentation

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Title: Structure and Evolution of Online Social Networks


1
Structure and Evolution of Online Social Networks
  • Ravi Kumar Jasmine Novak Andrew Tomkins

2
Our goal
  • To study real online social networks and answers
    questions like
  • How are social networks formed?
  • How do they evolve?
  • What properties do they exhibit?

3
Data Flickr and Yahoo! 360
  • Flickr (www.flickr.com)
  • online photo-sharing, social networking
  • graph nodes are users, edges friendships
  • 1M nodes, 8M directed edges
  • Yahoo! 360 (360.yahoo.com)
  • social networking website
  • graph nodes are users, edges are listed
    contacts
  • 5M nodes, 7M directed edges

4
Are friendships reciprocal in online social
networks?
  • 70 in Flickr and 84 in Yahoo! 360

5
How does density change with time?
6
Degree distribution Component size distribution
7
Segmenting the network three distinct regions
  • Singletons
  • degree-zero nodes who have joined the service,
    but have never connected to another user in the
    network
  • Giant component
  • densely connected core users, each connected to
    each other through paths in the social network
  • Middle region
  • remainder - isolated communities that connect to
    each other, but not the network at large

8
How do components merge as new links/nodes are
added in network?
9
Component sizes inFlickr Contacts
10
Component sizes in360 Contacts
11
How do components merge?
12
Surprising things about the Middle Region
  • These isolated communities account for a
    significant portion of the population 1/3 of
    Flickr, 1/10 of Yahoo! 360
  • Most of these components
  • form STARS! one or two
  • high-degree center nodes
  • connected to many low-degree twinkles
  • Despite growth (10x ) and dramatic changes in
    the particular users, the fraction of the
    population in isolated communities remains
    stable!

13
Characterizing the Stars in the middle region
14
How does the network diameter change with time?
15
The Giant Component
  • Do stars form the backbone of the GC?
  • No! Connectivity persists, even when stars and
    their twinkles are removed
  • How does it grow?
  • Do stars merge together to form bigger
    components, before finally joining the GC?
  • NO! Two processes dominate singletons joining
    the GC, and stars joining the GC
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